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NGC 2363, A Giant Extragalactic H II Region

Published online by Cambridge University Press:  04 August 2017

M. Peimbert ,
M. Peña  and
S. Torres-Peimbert
M. Peimbert
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México
M. Peña
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México
S. Torres-Peimbert
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México

Extract

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NGC 2363 is one of the extragalactic HII regions with the highest surface brightness in Hα and in λ5007. We discuss the physical conditions within this star-forming region. In particular, from spectrophometric studies in the 1200-7400 A range we have determined its chemical abundance. We find that the O/H is an order of magnitude smaller than in the solar vicinity, and that the C/O ratio is a factor of two smaller.

Type
II. Large Scale Processes of Star Formation
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 635 - 636
Copyright
Copyright © Reidel 1987