SciELO - Scientific Electronic Library Online

 
vol.43 número2Orbit, masses and spectral analysis of the visual binary a 2329Formation of a two-dense-rings-pattern disk from the collapse of a cloud índice de autoresíndice de assuntospesquisa de artigos
Home Pagelista alfabética de periódicos  

Serviços Personalizados

Journal

Artigo

Indicadores

Links relacionados

  • Não possue artigos similaresSimilares em SciELO

Compartilhar


Revista mexicana de astronomía y astrofísica

versão impressa ISSN 0185-1101

Resumo

MARTIN, M. C.; CAPPA, C. E.  e  TESTORI, J. C.. The neutral counterpart of an uncatalogued nebula and a probable interstellar bubble around wr 53 in the centaurus region. Rev. mex. astron. astrofis [online]. 2007, vol.43, n.2, pp.243-256. ISSN 0185-1101.

From the inspection of optical images at l = 307° we have found an uncata-logued nebula of about 9' in radius, which we named G307.27+0.27. The analysis of the HI-21cm line emission distribution revealed an expanding HI shell that encircles the optical emission region. The shell, placed at a kinematical distance of 4±1 kpc, is suggested to be the Hi counterpart of the optical nebula. CO observations at radio wavelengths, and far and mid IR data, allowed us to detect molecular gas and interstellar dust associated with the structures. The presence of an O6 star at a spectrophotometric distance compatible with that of the shell supports a stellar wind/HII region origin for the whole structure. We also report a probable Hi interstellar bubble related to the Wolf-Rayet star WR 53. Its physical parameters are similar to the parameters of other Hi bubbles around massive stars.

Palavras-chave : ISM; bubbles rayet-ISM; HII regions-stars; wolf-rayet.

        · resumo em Espanhol     · texto em Inglês

 

Creative Commons License Todo o conteúdo deste periódico, exceto onde está identificado, está licenciado sob uma Licença Creative Commons