Massive stars and their surrounding nebulae: A combined approach

S. Simón-Diáz; G. Stasińska; J. Garća-Rojas; C. Morisset; A. R. López-Sánchez; C. Esteban

Massive stars and their surrounding nebulae: A combined approach

S. Simón-Diáz^*, G. Stasińska, J. Garća-Rojas, C. Morisset, A. R. López-Sánchez, C. Esteban

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

1 Citation (Scopus)

Abstract

We present the first results of a project aimed at the combined study of massive stars and their surrounding nebulae by means of a detailed study of Galactic HII regions ionized by only one massive star. With this, we intend to check the validity of the new generation of massive star model atmosphere codes in terms of ionizing ux distribution. We take into account the effect of the nebular density distribution in our analyses. Various types of stellar and nebular observations have been collected for this purpose.

Original language	English
Pages (from-to)	137-139
Number of pages	3
Journal	Revista Mexicana de Astronomia y Astrofisica
Volume	33
Publication status	Published - 2008

Keywords

H II regions
ISM: individual (M 43)
ISM: ionization models
Stars: early-type
Stars: individual (HD 37061)

Cite this

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title = "Massive stars and their surrounding nebulae: A combined approach",

abstract = "We present the first results of a project aimed at the combined study of massive stars and their surrounding nebulae by means of a detailed study of Galactic HII regions ionized by only one massive star. With this, we intend to check the validity of the new generation of massive star model atmosphere codes in terms of ionizing ux distribution. We take into account the effect of the nebular density distribution in our analyses. Various types of stellar and nebular observations have been collected for this purpose.",

keywords = "H II regions, ISM: individual (M 43), ISM: ionization models, Stars: early-type, Stars: individual (HD 37061)",

author = "S. Sim{\'o}n-Di{\'a}z and G. Stasi{\'n}ska and J. Gar{\'c}a-Rojas and C. Morisset and L{\'o}pez-S{\'a}nchez, {A. R.} and C. Esteban",

year = "2008",

language = "English",

volume = "33",

pages = "137--139",

journal = "Revista Mexicana de Astronomia y Astrofisica",

issn = "0185-1101",

publisher = "Universidad Nacional Autonoma de Mexico",

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TY - JOUR

T1 - Massive stars and their surrounding nebulae

T2 - A combined approach

AU - Simón-Diáz, S.

AU - Stasińska, G.

AU - Garća-Rojas, J.

AU - Morisset, C.

AU - López-Sánchez, A. R.

AU - Esteban, C.

PY - 2008

Y1 - 2008

N2 - We present the first results of a project aimed at the combined study of massive stars and their surrounding nebulae by means of a detailed study of Galactic HII regions ionized by only one massive star. With this, we intend to check the validity of the new generation of massive star model atmosphere codes in terms of ionizing ux distribution. We take into account the effect of the nebular density distribution in our analyses. Various types of stellar and nebular observations have been collected for this purpose.

AB - We present the first results of a project aimed at the combined study of massive stars and their surrounding nebulae by means of a detailed study of Galactic HII regions ionized by only one massive star. With this, we intend to check the validity of the new generation of massive star model atmosphere codes in terms of ionizing ux distribution. We take into account the effect of the nebular density distribution in our analyses. Various types of stellar and nebular observations have been collected for this purpose.

KW - H II regions

KW - ISM: individual (M 43)

KW - ISM: ionization models

KW - Stars: early-type

KW - Stars: individual (HD 37061)

UR - http://www.scopus.com/inward/record.url?scp=72449149675&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:72449149675

SN - 0185-1101

VL - 33

SP - 137

EP - 139

JO - Revista Mexicana de Astronomia y Astrofisica

JF - Revista Mexicana de Astronomia y Astrofisica

ER -

Massive stars and their surrounding nebulae: A combined approach

Abstract

Keywords

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