The physical structure of Magellanic Cloud HII regions I. Dataset

R Vermeij; F Damour; JM van der Hulst; JP Baluteau

doi:10.1051/0004-6361:20020424

The physical structure of Magellanic Cloud HII regions I. Dataset

R Vermeij^*, F Damour, JM van der Hulst, JP Baluteau

^*Corresponding author for this work

Astronomy

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

33 Citations (Scopus)

Abstract

We present infrared and optical spectroscopic data for 11 H II regions and one Supernova Remnant in the Large and Small Magellanic Cloud. The infrared data have been obtained with the Short Wavelength Spectrometer and Long Wavelength Spectrometer on board the Infrared Space Observatory as part of a Guaranteed Time Program on H II regions in Local Group Galaxies. Aim of this project is to give a new and improved analysis of the physical structure of the sample H II regions by combining as much spectral data as possible. A detailed account is given here of the reduction process, and the quality and reliability of the presented fluxes are discussed.

Original language	English
Pages (from-to)	649-665
Number of pages	17
Journal	Astronomy & Astrophysics
Volume	390
Issue number	2
DOIs	https://doi.org/10.1051/0004-6361:20020424
Publication status	Published - Aug-2002

Keywords

ISM : lines and bands
HII regions
Magellanic Clouds
H-II REGIONS
30 DORADUS
WAVELENGTH SPECTROMETER
HST OBSERVATIONS
STELLAR CONTENT
LMC
STARS
SMC
30-DORADUS
BLOB

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@article{3d57534596164926851bc2648362ae23,

title = "The physical structure of Magellanic Cloud HII regions I. Dataset",

abstract = "We present infrared and optical spectroscopic data for 11 H II regions and one Supernova Remnant in the Large and Small Magellanic Cloud. The infrared data have been obtained with the Short Wavelength Spectrometer and Long Wavelength Spectrometer on board the Infrared Space Observatory as part of a Guaranteed Time Program on H II regions in Local Group Galaxies. Aim of this project is to give a new and improved analysis of the physical structure of the sample H II regions by combining as much spectral data as possible. A detailed account is given here of the reduction process, and the quality and reliability of the presented fluxes are discussed.",

keywords = "ISM : lines and bands, HII regions, Magellanic Clouds, H-II REGIONS, 30 DORADUS, WAVELENGTH SPECTROMETER, HST OBSERVATIONS, STELLAR CONTENT, LMC, STARS, SMC, 30-DORADUS, BLOB",

author = "R Vermeij and F Damour and {van der Hulst}, JM and JP Baluteau",

year = "2002",

month = aug,

doi = "10.1051/0004-6361:20020424",

language = "English",

volume = "390",

pages = "649--665",

journal = "Astronomy & Astrophysics",

issn = "0004-6361",

publisher = " EDP Sciences",

number = "2",

}

TY - JOUR

T1 - The physical structure of Magellanic Cloud HII regions I. Dataset

AU - Vermeij, R

AU - Damour, F

AU - van der Hulst, JM

AU - Baluteau, JP

PY - 2002/8

Y1 - 2002/8

N2 - We present infrared and optical spectroscopic data for 11 H II regions and one Supernova Remnant in the Large and Small Magellanic Cloud. The infrared data have been obtained with the Short Wavelength Spectrometer and Long Wavelength Spectrometer on board the Infrared Space Observatory as part of a Guaranteed Time Program on H II regions in Local Group Galaxies. Aim of this project is to give a new and improved analysis of the physical structure of the sample H II regions by combining as much spectral data as possible. A detailed account is given here of the reduction process, and the quality and reliability of the presented fluxes are discussed.

AB - We present infrared and optical spectroscopic data for 11 H II regions and one Supernova Remnant in the Large and Small Magellanic Cloud. The infrared data have been obtained with the Short Wavelength Spectrometer and Long Wavelength Spectrometer on board the Infrared Space Observatory as part of a Guaranteed Time Program on H II regions in Local Group Galaxies. Aim of this project is to give a new and improved analysis of the physical structure of the sample H II regions by combining as much spectral data as possible. A detailed account is given here of the reduction process, and the quality and reliability of the presented fluxes are discussed.

KW - ISM : lines and bands

KW - HII regions

KW - Magellanic Clouds

KW - H-II REGIONS

KW - 30 DORADUS

KW - WAVELENGTH SPECTROMETER

KW - HST OBSERVATIONS

KW - STELLAR CONTENT

KW - LMC

KW - STARS

KW - SMC

KW - 30-DORADUS

KW - BLOB

U2 - 10.1051/0004-6361:20020424

DO - 10.1051/0004-6361:20020424

M3 - Article

SN - 0004-6361

VL - 390

SP - 649

EP - 665

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

IS - 2

ER -

The physical structure of Magellanic Cloud HII regions I. Dataset

Abstract

Keywords

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