AustralieFrV1, PascalFrancis, Checkpoint, bibRecord, 004888

The giant pillars of the Carina Nebula

Identifieur interne : 004888 ( PascalFrancis/Checkpoint ); précédent : 004887; suivant : 004889

The giant pillars of the Carina Nebula

Auteurs : J. M. Rathborne [Chili, Australie, États-Unis] ; K. J. Brooks [Chili] ; M. G. Burton [Australie] ; M. Cohen [États-Unis] ; S. Bontemps [France]

Source :

Astronomy and astrophysics : (Berlin. Print) [ 0004-6361 ] ; 2004.

RBID : Pascal:04-0318877

Descripteurs français

Pascal (Inist)
- Carte radio, Continuum, Formation stellaire, Filament, Condensation, Vent stellaire, Rayonnement UV, Etoile proche, Etoile massive, Distribution densité, Objet stellaire jeune, Région H II compacte, Etoile OB, Région HII, Molécule interstellaire, Photodissociation.
Wicri :
- topic : Condensation.

English descriptors

KwdEn :
- Compact H II region, Continuum, Density distribution, Filaments, HII regions, Interstellar molecules, Massive stars, Nearby stars, OB stars, Photodissociation, Radio map, Star formation, Stellar winds, Ultraviolet radiation, Vapor condensation, Young stellar object.

Abstract

Results are presented from a multi-wavelength study of the giant pillars within the Carina Nebula. Using near-IR data from 2MASS, mid-IR data from MSX, 843 MHz radio continuum maps from the MOST and molecular line and continuum observations from the SEST, we investigate the nature of the pillars and search for evidence of ongoing star formation within them. Photodissociation regions (PDRs) exist across the whole nebula and trace the giant pillars, as well as many ridges, filaments and condensations (A_v > 7 mag). Morphological similarities between emission features at 21 μm and 843MHz adjacent to the PDRs, suggests that the molecular material has been carved by the intense stellar winds and UV radiation from the nearby massive stars. In addition, star forming cores are found at the tips of several of the pillars. Using a stellar density distribution, several candidate embedded clusters are also found. One is clearly seen in the 2MASS images and is located within a dense core (G287.84-0.82). A search for massive young stellar objects and compact H _II regions using mid-IR colour criteria, reveal twelve candidates across the complex. Grey-body fits to SEDs for four of these objects are suggestive of OB-stars. We find that massive star formation in the Carina Nebula is occurring across the whole complex and confirm it has been continuous over the past 3 Myrs.

Affiliations:

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Le document en format XML

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<front><div type="abstract" xml:lang="en">Results are presented from a multi-wavelength study of the giant pillars within the Carina Nebula. Using near-IR data from 2MASS, mid-IR data from MSX, 843 MHz radio continuum maps from the MOST and molecular line and continuum observations from the SEST, we investigate the nature of the pillars and search for evidence of ongoing star formation within them. Photodissociation regions (PDRs) exist across the whole nebula and trace the giant pillars, as well as many ridges, filaments and condensations (A<sub>v</sub>
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 regions using mid-IR colour criteria, reveal twelve candidates across the complex. Grey-body fits to SEDs for four of these objects are suggestive of OB-stars. We find that massive star formation in the Carina Nebula is occurring across the whole complex and confirm it has been continuous over the past 3 Myrs.</div>
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</fC03>
<fC03 i1="15" i2="3" l="ENG"><s0>Interstellar molecules</s0>
<s5>81</s5>
</fC03>
<fC03 i1="16" i2="3" l="FRE"><s0>Photodissociation</s0>
<s5>82</s5>
</fC03>
<fC03 i1="16" i2="3" l="ENG"><s0>Photodissociation</s0>
<s5>82</s5>
</fC03>
<fN21><s1>187</s1>
</fN21>
<fN44 i1="01"><s1>PSI</s1>
</fN44>
<fN82><s1>PSI</s1>
</fN82>
</pA>
</standard>
</inist>
<affiliations><list><country><li>Australie</li>
<li>Chili</li>
<li>France</li>
<li>États-Unis</li>
</country>
<region><li>Massachusetts</li>
</region>
<settlement><li>Boston</li>
</settlement>
</list>
<tree><country name="Chili"><noRegion><name sortKey="Rathborne, J M" sort="Rathborne, J M" uniqKey="Rathborne J" first="J. M." last="Rathborne">J. M. Rathborne</name>
</noRegion>
<name sortKey="Brooks, K J" sort="Brooks, K J" uniqKey="Brooks K" first="K. J." last="Brooks">K. J. Brooks</name>
<name sortKey="Brooks, K J" sort="Brooks, K J" uniqKey="Brooks K" first="K. J." last="Brooks">K. J. Brooks</name>
</country>
<country name="Australie"><noRegion><name sortKey="Rathborne, J M" sort="Rathborne, J M" uniqKey="Rathborne J" first="J. M." last="Rathborne">J. M. Rathborne</name>
</noRegion>
<name sortKey="Burton, M G" sort="Burton, M G" uniqKey="Burton M" first="M. G." last="Burton">M. G. Burton</name>
</country>
<country name="États-Unis"><region name="Massachusetts"><name sortKey="Rathborne, J M" sort="Rathborne, J M" uniqKey="Rathborne J" first="J. M." last="Rathborne">J. M. Rathborne</name>
</region>
<name sortKey="Cohen, M" sort="Cohen, M" uniqKey="Cohen M" first="M." last="Cohen">M. Cohen</name>
</country>
<country name="France"><noRegion><name sortKey="Bontemps, S" sort="Bontemps, S" uniqKey="Bontemps S" first="S." last="Bontemps">S. Bontemps</name>
</noRegion>
</country>
</tree>
</affiliations>
</record>

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{{Explor lien
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   |clé=     Pascal:04-0318877
   |texte=   The giant pillars of the Carina Nebula
}}

This area was generated with Dilib version V0.6.33.
Data generation: Tue Dec 5 10:43:12 2017. Site generation: Tue Mar 5 14:07:20 2024

	Serveur d'exploration sur les relations entre la France et l'Australie
	Attention, ce site est en cours de développement ! Attention, site généré par des moyens informatiques à partir de corpus bruts. Les informations ne sont donc pas validées.

Serveur d'exploration sur les relations entre la France et l'Australie

The giant pillars of the Carina Nebula

The giant pillars of the Carina Nebula

Source :

Descripteurs français

English descriptors

Abstract

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