Palabras clave
HII regions
ISM: jets and outflows
stars: pre-main sequence
stars: mass loss
ISM: jets and outflows
stars: pre-main sequence
stars: mass loss
Cómo citar
The new HI supershell GS263-02+45 and the OB Association Bochum 7: close relatives?. (2008). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 33, 160-160. https://astronomia.unam.mx/journals/rmxac/article/view/2008rmxac..33..160c
Resumen
Neutral hydrogen (HI) supershells are usually identified, in a given velocity range, as a brightness temperature minimum in the HI distribution that is surrounded by walls of HI emission. McClure-Griffiths et al. (2002) reported the discovery of GSH263+00+47, centered at (l,b) = (263°.0, 0°.0). The OB association Bochum 7 (l,b) = (265°.0, -2°.0) is seen in projection onto the outer border of GSH263+00+47 (see Figure 1).
Corti, M., Niemela, V., & Morrell, N. 2003, A&A, 405, 571
Corti, M. 2005, PhD Thesis, UNLP, Argentina
McClure-Griffiths, N. M., et al. 2002, ApJ, 578, 176
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