The environs of the H II region Gum 31
<b>Aims.</b> We analyze the distribution of the interstellar matter in the environs of the Hn region Gum 31, excited by the open cluster NGC 3324, located in the complex Carina region, with the aim of investigating the action of the massive stars on the surrounding neutral material. &l...
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| Autores principales: | , , , |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
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2008
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84886 |
| Aporte de: |
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I19-R120-10915-84886 |
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| record_format |
dspace |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Inglés |
| topic |
Ciencias Astronómicas ISM : bubbles ISM: Hn regions ISM: individual objects: Gum31 Stars: early-type Stars: individual: HD 92206 |
| spellingShingle |
Ciencias Astronómicas ISM : bubbles ISM: Hn regions ISM: individual objects: Gum31 Stars: early-type Stars: individual: HD 92206 Cappa, Cristina Elisabet Niemelä, Virpi Sinikka Amorín, R. Vasquez, Javier The environs of the H II region Gum 31 |
| topic_facet |
Ciencias Astronómicas ISM : bubbles ISM: Hn regions ISM: individual objects: Gum31 Stars: early-type Stars: individual: HD 92206 |
| description |
<b>Aims.</b> We analyze the distribution of the interstellar matter in the environs of the Hn region Gum 31, excited by the open cluster NGC 3324, located in the complex Carina region, with the aim of investigating the action of the massive stars on the surrounding neutral material.
<b>Methods.</b> We use neutral hydrogen 21-cm line data, radio continuum images at 0.843, 2.4 and 4.9 GHz, 12CO(1-0) observations, and IRAS and MSX infrared data.
<b>Results.</b> Adopting a distance of 3 kpc for the Hn region and the ionizing cluster, we derived an electron density of 33± 3 cm-3 and an ionized mass of (3.3 ±1.1) × 103 M⊙ based on the radio continuum data at 4.9 GHz. The Hl 21-cm line images revealed an Hl shell surrounding the Hn region. The Hl structure is 10.0 ±1.7 pc in radius, has a neutral mass of 1500 ±500 M⊙, and is expanding at 11 km s-1. The associated molecular gas amounts to (1.1 ±0.5) × 105 M⊙, being its volume density of about 350 cm-3. This molecular shell could represent the remains of the cloud where the young open cluster NGC 3324 was born or could have originated by the shock front associated with the Hn region. The difference between the ambient density and the electron density of the Hn region suggests that the Hn region is expanding. The distributions of the ionized and molecular material, along with that of the emission in the MSX band A, suggest that a photodissociation region has developed at the interface between the ionized and molecular gas. The copious UV photon flux from the early type stars in NGC 3324 keeps the Hn region ionized. The characteristics of a relatively large number of the IRAS, MSX, and 2MASS point sources projected onto the molecular envelope are compatible with protostellar candidates, showing the presence of active star forming regions. Very probably, the expansion of the Hn region has triggered stellar formation in the molecular shell. |
| format |
Articulo Articulo |
| author |
Cappa, Cristina Elisabet Niemelä, Virpi Sinikka Amorín, R. Vasquez, Javier |
| author_facet |
Cappa, Cristina Elisabet Niemelä, Virpi Sinikka Amorín, R. Vasquez, Javier |
| author_sort |
Cappa, Cristina Elisabet |
| title |
The environs of the H II region Gum 31 |
| title_short |
The environs of the H II region Gum 31 |
| title_full |
The environs of the H II region Gum 31 |
| title_fullStr |
The environs of the H II region Gum 31 |
| title_full_unstemmed |
The environs of the H II region Gum 31 |
| title_sort |
environs of the h ii region gum 31 |
| publishDate |
2008 |
| url |
http://sedici.unlp.edu.ar/handle/10915/84886 |
| work_keys_str_mv |
AT cappacristinaelisabet theenvironsofthehiiregiongum31 AT niemelavirpisinikka theenvironsofthehiiregiongum31 AT amorinr theenvironsofthehiiregiongum31 AT vasquezjavier theenvironsofthehiiregiongum31 AT cappacristinaelisabet environsofthehiiregiongum31 AT niemelavirpisinikka environsofthehiiregiongum31 AT amorinr environsofthehiiregiongum31 AT vasquezjavier environsofthehiiregiongum31 |
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Repositorios |
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1764820488677228544 |