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Cepheid investigations using the Kepler space telescope

Identifieur interne : 004215 ( PascalFrancis/Curation ); précédent : 004214; suivant : 004216

Cepheid investigations using the Kepler space telescope

Auteurs : R. Szabo [Hongrie] ; L. Szabados [Hongrie] ; C.-C. Ngeow [Taïwan] ; R. Smolec [Autriche] ; A. Derekas [Hongrie] ; P. Moskalik [Pologne] ; J. Nuspl [Hongrie] ; H. Lehmann [Allemagne] ; G. Füresz [États-Unis] ; J. Molenda-Zakowicz [Pologne] ; S. T. Bryson [États-Unis] ; A. A. Henden [États-Unis] ; D. W. Kurtz [Royaume-Uni] ; D. Stello [Australie] ; J. M. Nemec [Canada] ; J. M. Benkö [Hongrie] ; L. Berdnikov [Russie] ; H. Bruntt [France] ; N. R. Evans [États-Unis] ; N. A. Gorynya [Russie] ; E. N. Pastukhova [Russie] ; R. J. Simcoe [Russie] ; J. E. Grindlay [États-Unis] ; E. J. Los [États-Unis] ; A. Doane [États-Unis] ; S. G. Laycock [États-Unis] ; D. J. Mink [États-Unis] ; G. Champine [États-Unis] ; A. Sliski [États-Unis] ; G. Handler [Autriche] ; L. L. Kiss [Hongrie] ; Z. Kollath [Hongrie] ; J. Kovacs [Hongrie] ; J. Christensen-Dalsgaard [Danemark] ; H. Kjeldsen [Danemark] ; C. Allen [États-Unis] ; S. E. Thompson [États-Unis] ; J. Van Cleve [États-Unis]

Source :

RBID : Pascal:11-0253910

Descripteurs français

English descriptors

Abstract

We report results of initial work done on selected candidate Cepheids to be observed with the Kepler space telescope. Prior to the launch, 40 candidates were selected from previous surveys and data bases. The analysis of the first 322 d of Kepler photometry, and recent ground-based follow-up multicolour photometry and spectroscopy allowed us to confirm that one of these stars, V 1154 Cyg (KIC 7548061), is indeed a 4.9-d Cepheid. Using the phase lag method, we show that this star pulsates in the fundamental mode. New radial velocity data are consistent with previous measurements, suggesting that a long-period binary component is unlikely. No evidence is seen in the ultraprecise, nearly uninterrupted Kepler photometry for non-radial or stochastically excited modes at the micromagnitude level. The other candidates are not Cepheids, but an interesting mix of possible spotted stars, eclipsing systems and flare stars.
pA  
A01 01  1    @0 0035-8711
A02 01      @0 MNRAA4
A03   1    @0 Mon. Not. R. Astron. Soc.
A05       @2 413
A06       @2 4
A08 01  1  ENG  @1 Cepheid investigations using the Kepler space telescope
A11 01  1    @1 SZABO (R.)
A11 02  1    @1 SZABADOS (L.)
A11 03  1    @1 NGEOW (C.-C.)
A11 04  1    @1 SMOLEC (R.)
A11 05  1    @1 DEREKAS (A.)
A11 06  1    @1 MOSKALIK (P.)
A11 07  1    @1 NUSPL (J.)
A11 08  1    @1 LEHMANN (H.)
A11 09  1    @1 FÜRESZ (G.)
A11 10  1    @1 MOLENDA-ZAKOWICZ (J.)
A11 11  1    @1 BRYSON (S. T.)
A11 12  1    @1 HENDEN (A. A.)
A11 13  1    @1 KURTZ (D. W.)
A11 14  1    @1 STELLO (D.)
A11 15  1    @1 NEMEC (J. M.)
A11 16  1    @1 BENKÖ (J. M.)
A11 17  1    @1 BERDNIKOV (L.)
A11 18  1    @1 BRUNTT (H.)
A11 19  1    @1 EVANS (N. R.)
A11 20  1    @1 GORYNYA (N. A.)
A11 21  1    @1 PASTUKHOVA (E. N.)
A11 22  1    @1 SIMCOE (R. J.)
A11 23  1    @1 GRINDLAY (J. E.)
A11 24  1    @1 LOS (E. J.)
A11 25  1    @1 DOANE (A.)
A11 26  1    @1 LAYCOCK (S. G.)
A11 27  1    @1 MINK (D. J.)
A11 28  1    @1 CHAMPINE (G.)
A11 29  1    @1 SLISKI (A.)
A11 30  1    @1 HANDLER (G.)
A11 31  1    @1 KISS (L. L.)
A11 32  1    @1 KOLLATH (Z.)
A11 33  1    @1 KOVACS (J.)
A11 34  1    @1 CHRISTENSEN-DALSGAARD (J.)
A11 35  1    @1 KJELDSEN (H.)
A11 36  1    @1 ALLEN (C.)
A11 37  1    @1 THOMPSON (S. E.)
A11 38  1    @1 VAN CLEVE (J.)
A14 01      @1 Konkoly Observatory of the Hungarian Academy of Sciences, Konkoly Thege Miklós út 15-17 @2 1121 Budapest @3 HUN @Z 1 aut. @Z 2 aut. @Z 5 aut. @Z 7 aut. @Z 16 aut. @Z 31 aut. @Z 32 aut.
A14 02      @1 Graduate Institute of Astronomy, National Central University @2 Jhongli City, Taoyuan County 32001 @3 TWN @Z 3 aut.
A14 03      @1 Institut für Astronomie, Universität Wien, Türkenschanzstrasse 17 @2 1180 Wien @3 AUT @Z 4 aut. @Z 30 aut.
A14 04      @1 Department of Astronomy, Eötvös University @2 Budapest @3 HUN @Z 5 aut.
A14 05      @1 Copernicus Astronomical Center, ul. Bartycka 18 @2 00-716 Warsaw @3 POL @Z 6 aut.
A14 06      @1 Thüringer Landessternwarte Tautenburg, Karl-Schwarzschild-Observatorium @2 07778 Tautenburg @3 DEU @Z 8 aut.
A14 07      @1 Harvard-Smithsonian Center for Astrophysics, MS 20, 60 Garden Street @2 Cambridge, MA 02138 @3 USA @Z 9 aut.
A14 08      @1 Astronomical Institute, University of Wroclaw, ul. Kopernika 11 @2 51-622 Wroclaw @3 POL @Z 10 aut.
A14 09      @1 NASA Ames Research Center @2 Moffett Field, CA 94035 @3 USA @Z 11 aut.
A14 10      @1 American Association of Variable Star Observers @2 Cambridge, MA 02138 @3 USA @Z 12 aut.
A14 11      @1 Jeremiah Horrocks Institute of Astrophysics, University of Central Lancashire @2 Preston PRI 2HE @3 GBR @Z 13 aut.
A14 12      @1 Sydney Institute for Astronomy, School of Physics, The University of Sydney @2 Sydney, 2006 NSW @3 AUS @Z 14 aut.
A14 13      @1 Department of Physics & Astronomy, Camosun College @2 Victoria, British Columbia V8P 5J2 @3 CAN @Z 15 aut.
A14 14      @1 Sternberg Astronomical Institute, Moscow University @2 Moscow @3 RUS @Z 17 aut. @Z 22 aut.
A14 15      @1 Isaac Newton Institute of Chile, Moscow Branch, Universitetskij Pr. 13 @2 Moscow 119992 @3 RUS @Z 17 aut.
A14 16      @1 LESIA, UMR 8109, Observatoire de Paris @2 92195 Meudon @3 FRA @Z 18 aut.
A14 17      @1 Smithsonian Astrophysical Observatory, MS 4, 60 Garden Street @2 Cambridge, MA 02138 @3 USA @Z 19 aut. @Z 27 aut.
A14 18      @1 Institute of Astronomy, Russian Academy of Sciences, 48 Pyatnitskaya Street @2 Moscow 109017 @3 RUS @Z 20 aut. @Z 21 aut.
A14 19      @1 Harvard College Observatory, 60 Garden Street @2 Cambridge, MA 02138 @3 USA @Z 23 aut. @Z 24 aut. @Z 25 aut. @Z 26 aut. @Z 28 aut. @Z 29 aut.
A14 20      @1 Gothard Astrophysical Observatory @2 9707 Szombathely @3 HUN @Z 33 aut.
A14 21      @1 Department of Physics and Astronomy, Aarhus University @2 8000 Aarhus @3 DNK @Z 34 aut. @Z 35 aut.
A14 22      @1 Orbital Sciences Corporntion/NASA Ames Research Center @2 Moffett Field, CA 94035 @3 USA @Z 36 aut.
A14 23      @1 SET1 Institute/NASA Ames Research Center @2 Moffett Field, CA 94035 @3 USA @Z 37 aut. @Z 38 aut.
A20       @1 2709-2720
A21       @1 2011
A23 01      @0 ENG
A43 01      @1 INIST @2 2067 @5 354000191585840350
A44       @0 0000 @1 © 2011 INIST-CNRS. All rights reserved.
A45       @0 3/4 p.
A47 01  1    @0 11-0253910
A60       @1 P
A61       @0 A
A64 01  1    @0 Monthly Notices of the Royal Astronomical Society
A66 01      @0 USA
C01 01    ENG  @0 We report results of initial work done on selected candidate Cepheids to be observed with the Kepler space telescope. Prior to the launch, 40 candidates were selected from previous surveys and data bases. The analysis of the first 322 d of Kepler photometry, and recent ground-based follow-up multicolour photometry and spectroscopy allowed us to confirm that one of these stars, V 1154 Cyg (KIC 7548061), is indeed a 4.9-d Cepheid. Using the phase lag method, we show that this star pulsates in the fundamental mode. New radial velocity data are consistent with previous measurements, suggesting that a long-period binary component is unlikely. No evidence is seen in the ultraprecise, nearly uninterrupted Kepler photometry for non-radial or stochastically excited modes at the micromagnitude level. The other candidates are not Cepheids, but an interesting mix of possible spotted stars, eclipsing systems and flare stars.
C02 01  3    @0 001E03
C03 01  3  FRE  @0 Céphéide @5 26
C03 01  3  ENG  @0 Cepheids @5 26
C03 02  X  FRE  @0 Photométrie n couleurs @5 27
C03 02  X  ENG  @0 N color photometry @5 27
C03 02  X  SPA  @0 Fotometría n colores @5 27
C03 03  3  FRE  @0 Spectrométrie @5 28
C03 03  3  ENG  @0 Spectroscopy @5 28
C03 04  3  FRE  @0 Vitesse radiale @5 29
C03 04  3  ENG  @0 Radial velocity @5 29
C03 05  3  FRE  @0 Etoile à sursauts @5 30
C03 05  3  ENG  @0 Flare stars @5 30
N21       @1 171
N44 01      @1 OTO
N82       @1 OTO

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<name sortKey="Simcoe, R J" sort="Simcoe, R J" uniqKey="Simcoe R" first="R. J." last="Simcoe">R. J. Simcoe</name>
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<name sortKey="Grindlay, J E" sort="Grindlay, J E" uniqKey="Grindlay J" first="J. E." last="Grindlay">J. E. Grindlay</name>
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<inist:fA14 i1="20">
<s1>Gothard Astrophysical Observatory</s1>
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<country>Hongrie</country>
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<name sortKey="Christensen Dalsgaard, J" sort="Christensen Dalsgaard, J" uniqKey="Christensen Dalsgaard J" first="J." last="Christensen-Dalsgaard">J. Christensen-Dalsgaard</name>
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<s1>Department of Physics and Astronomy, Aarhus University</s1>
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<sZ>34 aut.</sZ>
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<s1>SET1 Institute/NASA Ames Research Center</s1>
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<inist:fA14 i1="23">
<s1>SET1 Institute/NASA Ames Research Center</s1>
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<title xml:lang="en" level="a">Cepheid investigations using the Kepler space telescope</title>
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<inist:fA14 i1="01">
<s1>Konkoly Observatory of the Hungarian Academy of Sciences, Konkoly Thege Miklós út 15-17</s1>
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<s3>HUN</s3>
<sZ>1 aut.</sZ>
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<country>Hongrie</country>
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<author>
<name sortKey="Szabados, L" sort="Szabados, L" uniqKey="Szabados L" first="L." last="Szabados">L. Szabados</name>
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<inist:fA14 i1="01">
<s1>Konkoly Observatory of the Hungarian Academy of Sciences, Konkoly Thege Miklós út 15-17</s1>
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<s3>HUN</s3>
<sZ>1 aut.</sZ>
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<name sortKey="Ngeow, C C" sort="Ngeow, C C" uniqKey="Ngeow C" first="C.-C." last="Ngeow">C.-C. Ngeow</name>
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<inist:fA14 i1="02">
<s1>Graduate Institute of Astronomy, National Central University</s1>
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<name sortKey="Smolec, R" sort="Smolec, R" uniqKey="Smolec R" first="R." last="Smolec">R. Smolec</name>
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<inist:fA14 i1="04">
<s1>Department of Astronomy, Eötvös University</s1>
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<sZ>5 aut.</sZ>
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<name sortKey="Moskalik, P" sort="Moskalik, P" uniqKey="Moskalik P" first="P." last="Moskalik">P. Moskalik</name>
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<s1>Copernicus Astronomical Center, ul. Bartycka 18</s1>
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<s1>Konkoly Observatory of the Hungarian Academy of Sciences, Konkoly Thege Miklós út 15-17</s1>
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<inist:fA14 i1="06">
<s1>Thüringer Landessternwarte Tautenburg, Karl-Schwarzschild-Observatorium</s1>
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<country>Allemagne</country>
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<name sortKey="Furesz, G" sort="Furesz, G" uniqKey="Furesz G" first="G." last="Füresz">G. Füresz</name>
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<inist:fA14 i1="07">
<s1>Harvard-Smithsonian Center for Astrophysics, MS 20, 60 Garden Street</s1>
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<name sortKey="Molenda Zakowicz, J" sort="Molenda Zakowicz, J" uniqKey="Molenda Zakowicz J" first="J." last="Molenda-Zakowicz">J. Molenda-Zakowicz</name>
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<inist:fA14 i1="08">
<s1>Astronomical Institute, University of Wroclaw, ul. Kopernika 11</s1>
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<name sortKey="Bryson, S T" sort="Bryson, S T" uniqKey="Bryson S" first="S. T." last="Bryson">S. T. Bryson</name>
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<inist:fA14 i1="09">
<s1>NASA Ames Research Center</s1>
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<name sortKey="Henden, A A" sort="Henden, A A" uniqKey="Henden A" first="A. A." last="Henden">A. A. Henden</name>
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<inist:fA14 i1="10">
<s1>American Association of Variable Star Observers</s1>
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<name sortKey="Kurtz, D W" sort="Kurtz, D W" uniqKey="Kurtz D" first="D. W." last="Kurtz">D. W. Kurtz</name>
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<inist:fA14 i1="11">
<s1>Jeremiah Horrocks Institute of Astrophysics, University of Central Lancashire</s1>
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<name sortKey="Stello, D" sort="Stello, D" uniqKey="Stello D" first="D." last="Stello">D. Stello</name>
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<inist:fA14 i1="12">
<s1>Sydney Institute for Astronomy, School of Physics, The University of Sydney</s1>
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<inist:fA14 i1="13">
<s1>Department of Physics & Astronomy, Camosun College</s1>
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<name sortKey="Benko, J M" sort="Benko, J M" uniqKey="Benko J" first="J. M." last="Benkö">J. M. Benkö</name>
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<s1>Konkoly Observatory of the Hungarian Academy of Sciences, Konkoly Thege Miklós út 15-17</s1>
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<inist:fA14 i1="15">
<s1>Isaac Newton Institute of Chile, Moscow Branch, Universitetskij Pr. 13</s1>
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<name sortKey="Bruntt, H" sort="Bruntt, H" uniqKey="Bruntt H" first="H." last="Bruntt">H. Bruntt</name>
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<inist:fA14 i1="16">
<s1>LESIA, UMR 8109, Observatoire de Paris</s1>
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<name sortKey="Evans, N R" sort="Evans, N R" uniqKey="Evans N" first="N. R." last="Evans">N. R. Evans</name>
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<name sortKey="Pastukhova, E N" sort="Pastukhova, E N" uniqKey="Pastukhova E" first="E. N." last="Pastukhova">E. N. Pastukhova</name>
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<s1>Institute of Astronomy, Russian Academy of Sciences, 48 Pyatnitskaya Street</s1>
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<name sortKey="Simcoe, R J" sort="Simcoe, R J" uniqKey="Simcoe R" first="R. J." last="Simcoe">R. J. Simcoe</name>
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<name sortKey="Mink, D J" sort="Mink, D J" uniqKey="Mink D" first="D. J." last="Mink">D. J. Mink</name>
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<name sortKey="Champine, G" sort="Champine, G" uniqKey="Champine G" first="G." last="Champine">G. Champine</name>
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<name sortKey="Sliski, A" sort="Sliski, A" uniqKey="Sliski A" first="A." last="Sliski">A. Sliski</name>
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<name sortKey="Handler, G" sort="Handler, G" uniqKey="Handler G" first="G." last="Handler">G. Handler</name>
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<country>Autriche</country>
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<name sortKey="Kiss, L L" sort="Kiss, L L" uniqKey="Kiss L" first="L. L." last="Kiss">L. L. Kiss</name>
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<country>Hongrie</country>
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<name sortKey="Kovacs, J" sort="Kovacs, J" uniqKey="Kovacs J" first="J." last="Kovacs">J. Kovacs</name>
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<country>Hongrie</country>
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</author>
<author>
<name sortKey="Christensen Dalsgaard, J" sort="Christensen Dalsgaard, J" uniqKey="Christensen Dalsgaard J" first="J." last="Christensen-Dalsgaard">J. Christensen-Dalsgaard</name>
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<s1>Department of Physics and Astronomy, Aarhus University</s1>
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<country>Danemark</country>
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<name sortKey="Kjeldsen, H" sort="Kjeldsen, H" uniqKey="Kjeldsen H" first="H." last="Kjeldsen">H. Kjeldsen</name>
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<author>
<name sortKey="Allen, C" sort="Allen, C" uniqKey="Allen C" first="C." last="Allen">C. Allen</name>
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</author>
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<name sortKey="Thompson, S E" sort="Thompson, S E" uniqKey="Thompson S" first="S. E." last="Thompson">S. E. Thompson</name>
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<author>
<name sortKey="Van Cleve, J" sort="Van Cleve, J" uniqKey="Van Cleve J" first="J." last="Van Cleve">J. Van Cleve</name>
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<series>
<title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title>
<title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title>
<idno type="ISSN">0035-8711</idno>
<imprint>
<date when="2011">2011</date>
</imprint>
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<title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title>
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<keywords scheme="KwdEn" xml:lang="en">
<term>Cepheids</term>
<term>Flare stars</term>
<term>N color photometry</term>
<term>Radial velocity</term>
<term>Spectroscopy</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Céphéide</term>
<term>Photométrie n couleurs</term>
<term>Spectrométrie</term>
<term>Vitesse radiale</term>
<term>Etoile à sursauts</term>
</keywords>
<keywords scheme="Wicri" type="topic" xml:lang="fr">
<term>Spectrométrie</term>
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<front>
<div type="abstract" xml:lang="en">We report results of initial work done on selected candidate Cepheids to be observed with the Kepler space telescope. Prior to the launch, 40 candidates were selected from previous surveys and data bases. The analysis of the first 322 d of Kepler photometry, and recent ground-based follow-up multicolour photometry and spectroscopy allowed us to confirm that one of these stars, V 1154 Cyg (KIC 7548061), is indeed a 4.9-d Cepheid. Using the phase lag method, we show that this star pulsates in the fundamental mode. New radial velocity data are consistent with previous measurements, suggesting that a long-period binary component is unlikely. No evidence is seen in the ultraprecise, nearly uninterrupted Kepler photometry for non-radial or stochastically excited modes at the micromagnitude level. The other candidates are not Cepheids, but an interesting mix of possible spotted stars, eclipsing systems and flare stars.</div>
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<s1>CHRISTENSEN-DALSGAARD (J.)</s1>
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<s1>Department of Astronomy, Eötvös University</s1>
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<fA14 i1="05">
<s1>Copernicus Astronomical Center, ul. Bartycka 18</s1>
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<fA14 i1="06">
<s1>Thüringer Landessternwarte Tautenburg, Karl-Schwarzschild-Observatorium</s1>
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<fA14 i1="07">
<s1>Harvard-Smithsonian Center for Astrophysics, MS 20, 60 Garden Street</s1>
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<fA14 i1="08">
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<s1>NASA Ames Research Center</s1>
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<fA14 i1="10">
<s1>American Association of Variable Star Observers</s1>
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<sZ>12 aut.</sZ>
</fA14>
<fA14 i1="11">
<s1>Jeremiah Horrocks Institute of Astrophysics, University of Central Lancashire</s1>
<s2>Preston PRI 2HE</s2>
<s3>GBR</s3>
<sZ>13 aut.</sZ>
</fA14>
<fA14 i1="12">
<s1>Sydney Institute for Astronomy, School of Physics, The University of Sydney</s1>
<s2>Sydney, 2006 NSW</s2>
<s3>AUS</s3>
<sZ>14 aut.</sZ>
</fA14>
<fA14 i1="13">
<s1>Department of Physics & Astronomy, Camosun College</s1>
<s2>Victoria, British Columbia V8P 5J2</s2>
<s3>CAN</s3>
<sZ>15 aut.</sZ>
</fA14>
<fA14 i1="14">
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<sZ>17 aut.</sZ>
<sZ>22 aut.</sZ>
</fA14>
<fA14 i1="15">
<s1>Isaac Newton Institute of Chile, Moscow Branch, Universitetskij Pr. 13</s1>
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<sZ>17 aut.</sZ>
</fA14>
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<s1>LESIA, UMR 8109, Observatoire de Paris</s1>
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<fA14 i1="17">
<s1>Smithsonian Astrophysical Observatory, MS 4, 60 Garden Street</s1>
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<sZ>19 aut.</sZ>
<sZ>27 aut.</sZ>
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<fA14 i1="18">
<s1>Institute of Astronomy, Russian Academy of Sciences, 48 Pyatnitskaya Street</s1>
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<s3>RUS</s3>
<sZ>20 aut.</sZ>
<sZ>21 aut.</sZ>
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<fA14 i1="19">
<s1>Harvard College Observatory, 60 Garden Street</s1>
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<sZ>24 aut.</sZ>
<sZ>25 aut.</sZ>
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<s0>A</s0>
</fA61>
<fA64 i1="01" i2="1">
<s0>Monthly Notices of the Royal Astronomical Society</s0>
</fA64>
<fA66 i1="01">
<s0>USA</s0>
</fA66>
<fC01 i1="01" l="ENG">
<s0>We report results of initial work done on selected candidate Cepheids to be observed with the Kepler space telescope. Prior to the launch, 40 candidates were selected from previous surveys and data bases. The analysis of the first 322 d of Kepler photometry, and recent ground-based follow-up multicolour photometry and spectroscopy allowed us to confirm that one of these stars, V 1154 Cyg (KIC 7548061), is indeed a 4.9-d Cepheid. Using the phase lag method, we show that this star pulsates in the fundamental mode. New radial velocity data are consistent with previous measurements, suggesting that a long-period binary component is unlikely. No evidence is seen in the ultraprecise, nearly uninterrupted Kepler photometry for non-radial or stochastically excited modes at the micromagnitude level. The other candidates are not Cepheids, but an interesting mix of possible spotted stars, eclipsing systems and flare stars.</s0>
</fC01>
<fC02 i1="01" i2="3">
<s0>001E03</s0>
</fC02>
<fC03 i1="01" i2="3" l="FRE">
<s0>Céphéide</s0>
<s5>26</s5>
</fC03>
<fC03 i1="01" i2="3" l="ENG">
<s0>Cepheids</s0>
<s5>26</s5>
</fC03>
<fC03 i1="02" i2="X" l="FRE">
<s0>Photométrie n couleurs</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="X" l="ENG">
<s0>N color photometry</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="X" l="SPA">
<s0>Fotometría n colores</s0>
<s5>27</s5>
</fC03>
<fC03 i1="03" i2="3" l="FRE">
<s0>Spectrométrie</s0>
<s5>28</s5>
</fC03>
<fC03 i1="03" i2="3" l="ENG">
<s0>Spectroscopy</s0>
<s5>28</s5>
</fC03>
<fC03 i1="04" i2="3" l="FRE">
<s0>Vitesse radiale</s0>
<s5>29</s5>
</fC03>
<fC03 i1="04" i2="3" l="ENG">
<s0>Radial velocity</s0>
<s5>29</s5>
</fC03>
<fC03 i1="05" i2="3" l="FRE">
<s0>Etoile à sursauts</s0>
<s5>30</s5>
</fC03>
<fC03 i1="05" i2="3" l="ENG">
<s0>Flare stars</s0>
<s5>30</s5>
</fC03>
<fN21>
<s1>171</s1>
</fN21>
<fN44 i1="01">
<s1>OTO</s1>
</fN44>
<fN82>
<s1>OTO</s1>
</fN82>
</pA>
</standard>
</inist>
</record>

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