A search for millimeter wave spectral lines from comet Sugano-Saigusa-Fujikawa (1983e)
Identifieur interne : 004079 ( Main/Merge ); précédent : 004078; suivant : 004080A search for millimeter wave spectral lines from comet Sugano-Saigusa-Fujikawa (1983e)
Auteurs : Tetsuo Hasegawa [Japon] ; Masatoshi Ohishi [Japon] ; Masaki Morimoto [Japon] ; Hiroko Suzuki [Japon] ; Norio Kaifu [Japon]Source :
- Icarus [ 0019-1035 ] ; 1984.
Abstract
The search for radio spectral lines from Comet Sugano-Saigusa-Fujikawa (1983e) was conducted using the 45-m telescope of Nobeyama Radio Observatory. The frequency ranges of 44.0–46.0 and 47.5–49.5 GHz were surveyed down to ΔTA∗ (rms) = 20–30 mK, with a beam size of ∼35 arc sec. Upper limits have been established for spectral lines of atomic hydrogen, CS, OCS, SO2, H2CO, CH3OH, HCCCCCN, HCOOCH3, CH3OCH3, and CH3CH2CN. The J = 5−4 line from HCCCN in the vibrational ground state possibly has been detected but not confirmed. The suggested total amount of HCCCN in the coma is consistent with the possible picture that HCCCN is the main parent molecule of CN.
Url:
DOI: 10.1016/0019-1035(84)90149-0
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384-13</wicri:noRegion></affiliation></author></analytic><monogr></monogr><series><title level="j">Icarus</title><title level="j" type="abbrev">YICAR</title><idno type="ISSN">0019-1035</idno><imprint><publisher>ELSEVIER</publisher><date type="published" when="1984">1984</date><biblScope unit="volume">60</biblScope><biblScope unit="issue">1</biblScope><biblScope unit="page" from="211">211</biblScope><biblScope unit="page" to="214">214</biblScope></imprint><idno type="ISSN">0019-1035</idno></series><idno type="istex">7C540FA4A89CA9AB38F0EC0F5D6B9939EEE14FA3</idno><idno type="DOI">10.1016/0019-1035(84)90149-0</idno><idno type="PII">0019-1035(84)90149-0</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0019-1035</idno></seriesStmt></fileDesc><profileDesc><textClass></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">The search for radio spectral lines from Comet Sugano-Saigusa-Fujikawa (1983e) was conducted using the 45-m telescope of Nobeyama Radio Observatory. The frequency ranges of 44.0–46.0 and 47.5–49.5 GHz were surveyed down to ΔTA∗ (rms) = 20–30 mK, with a beam size of ∼35 arc sec. Upper limits have been established for spectral lines of atomic hydrogen, CS, OCS, SO2, H2CO, CH3OH, HCCCCCN, HCOOCH3, CH3OCH3, and CH3CH2CN. The J = 5−4 line from HCCCN in the vibrational ground state possibly has been detected but not confirmed. The suggested total amount of HCCCN in the coma is consistent with the possible picture that HCCCN is the main parent molecule of CN.</div></front></TEI></record>Pour manipuler ce document sous Unix (Dilib)
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