AustralieFrV1, Main, Exploration, bibRecord, 006D93

A detailed study of the H II region M 43 and its ionizing star I. Stellar parameters and nebular empirical analysis

Identifieur interne : 006D93 ( Main/Exploration ); précédent : 006D92; suivant : 006D94

A detailed study of the H II region M 43 and its ionizing star I. Stellar parameters and nebular empirical analysis

Auteurs : S. Simon-Diaz [Espagne] ; J. Garcia-Rojas [Espagne, Mexique] ; C. Esteban [Espagne] ; G. Stasinska [France] ; A. R. Lopez-Sanchez [Australie] ; C. Morisset [Mexique]

Source :

Astronomy and astrophysics : (Berlin. Print) [ 0004-6361 ] ; 2011.

RBID : Pascal:11-0447973

Descripteurs français

Pascal (Inist)
- Région HII, Etoile excitatrice, Paramètre physique, Etoile massive, Spectre optique, Spectrométrie, Photoionisation, Modèle, Lumière diffuse, Nébuleuse Orion, Correction, Observation spectroscopique, Luminosité, Abondance, Répartition spatiale, Ionisation, Etoile premier type, Matière circumstellaire.
Wicri :
- topic : Spectrométrie.

English descriptors

KwdEn :
- Abundance, Circumstellar matter, Corrections, Early type stars, Exciting star, HII regions, Ionization, Luminosity, Massive stars, Models, Optical spectrum, Orion nebula, Photoionization, Physical parameter, Scattered light, Spatial distribution, Spectroscopical observation, Spectroscopy.

Abstract

Aims. We have selected the Galactic H II region M 43, a close-by apparently spherical nebula ionized by a single star (HD 37061, B0.5 V) to investigate several topics of recent interest in the field of H II regions and massive stars. In a series of two papers, we perform a combined, comprehensive study of the nebula and its ionizing star by using as many observational constraints as possible. Methods. We collected for this study a set of high-quality observations, including the optical spectrum of HD 37061, along with nebular optical imaging and long-slit spatially resolved spectroscopy. The first part of our study comprises a quantitative spectroscopic analysis of the ionizing star, and the empirical analysis of the nebular images and spectroscopy. All the information obtained here will be used to construct a customised photoionization model of the nebula in Paper II. Results. We determine the stellar parameters of HD 37061 and the total number of ionizing photons emitted by the star. We find observational evidence of scattered light from the Huygens region (the brightest part of the Orion nebula) in the M 43 region. We show the importance of an adequate correction of this scattered light in both the imagery and spectroscopic observations of M 43 in accurately determining the total nebular Hα luminosity, the nebular physical conditions. and chemical abundances. We perform a detailed nebular empirical analysis of nine apertures extracted from a long-slit located to the west of HD 37061 (east-west direction), obtaining the spatial distribution of the physical conditions and ionic abundances. For three of the analyzed elements (O, S, and N), we determine total abundances directly from observable ions (no ionization correction factors are needed). The comparison of these abundances with those derived from the spectrum of the Orion nebula indicates the importance of the atomic data and, specially in the case of M 42, the considered ionization correction factors.

Affiliations:

Australie, Espagne, France, Mexique

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Le document en format XML

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<term>Etoile massive</term>
<term>Spectre optique</term>
<term>Spectrométrie</term>
<term>Photoionisation</term>
<term>Modèle</term>
<term>Lumière diffuse</term>
<term>Nébuleuse Orion</term>
<term>Correction</term>
<term>Observation spectroscopique</term>
<term>Luminosité</term>
<term>Abondance</term>
<term>Répartition spatiale</term>
<term>Ionisation</term>
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<front><div type="abstract" xml:lang="en">Aims. We have selected the Galactic H II region M 43, a close-by apparently spherical nebula ionized by a single star (HD 37061, B0.5 V) to investigate several topics of recent interest in the field of H II regions and massive stars. In a series of two papers, we perform a combined, comprehensive study of the nebula and its ionizing star by using as many observational constraints as possible. Methods. We collected for this study a set of high-quality observations, including the optical spectrum of HD 37061, along with nebular optical imaging and long-slit spatially resolved spectroscopy. The first part of our study comprises a quantitative spectroscopic analysis of the ionizing star, and the empirical analysis of the nebular images and spectroscopy. All the information obtained here will be used to construct a customised photoionization model of the nebula in Paper II. Results. We determine the stellar parameters of HD 37061 and the total number of ionizing photons emitted by the star. We find observational evidence of scattered light from the Huygens region (the brightest part of the Orion nebula) in the M 43 region. We show the importance of an adequate correction of this scattered light in both the imagery and spectroscopic observations of M 43 in accurately determining the total nebular Hα luminosity, the nebular physical conditions. and chemical abundances. We perform a detailed nebular empirical analysis of nine apertures extracted from a long-slit located to the west of HD 37061 (east-west direction), obtaining the spatial distribution of the physical conditions and ionic abundances. For three of the analyzed elements (O, S, and N), we determine total abundances directly from observable ions (no ionization correction factors are needed). The comparison of these abundances with those derived from the spectrum of the Orion nebula indicates the importance of the atomic data and, specially in the case of M 42, the considered ionization correction factors.</div>
</front>
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A detailed study of the H II region M 43 and its ionizing star I. Stellar parameters and nebular empirical analysis

A detailed study of the H II region M 43 and its ionizing star I. Stellar parameters and nebular empirical analysis

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Descripteurs français

English descriptors

Abstract

Links toward previous steps (curation, corpus...)

Le document en format XML

Pour manipuler ce document sous Unix (Dilib)

Pour mettre un lien sur cette page dans le réseau Wicri