Abstract
IRAS far-infrared fluxes are presented for six H II regions in the Large Magellanic Cloud. These regions are the sites of recent, massive star formation where the radiative heating source is young stars rather than the general interstellar radiation field. As such, the observations become building blocks for the interpretation of far-infrared emission from spatially unresolved galaxies. In addition, the multiwavelength luminosities of the region then probe the young stellar upper initial mass function. With the long-range goal of determining the stellar content of unresolved star-forming regions, we present the results of a simple model which combines the infrared data with existing Hα/Hβ and thermal radio data. For the two OB associations where the mass function has been determined directly, the model correctly "predicts" a solar neighborhood upper mass function within the uncertainties. No evidence is found for upper mass functions significantly different from that in the solar neighborhood.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 542-551 |
| Number of pages | 10 |
| Journal | Astrophysical Journal |
| Volume | 397 |
| Issue number | 2 |
| State | Published - 1992 |
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Keywords
- H II regions
- Infrared: interstellar: continuum
- Magellanic Clouds
- Stars: formation
ASJC Scopus subject areas
- Space and Planetary Science
Cite this
IRAS observations and the stellar content of H II regions in the large magellanic cloud. / Eastwood, Kathleen D.
In: Astrophysical Journal, Vol. 397, No. 2, 1992, p. 542-551.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - IRAS observations and the stellar content of H II regions in the large magellanic cloud
AU - Eastwood, Kathleen D
PY - 1992
Y1 - 1992
N2 - IRAS far-infrared fluxes are presented for six H II regions in the Large Magellanic Cloud. These regions are the sites of recent, massive star formation where the radiative heating source is young stars rather than the general interstellar radiation field. As such, the observations become building blocks for the interpretation of far-infrared emission from spatially unresolved galaxies. In addition, the multiwavelength luminosities of the region then probe the young stellar upper initial mass function. With the long-range goal of determining the stellar content of unresolved star-forming regions, we present the results of a simple model which combines the infrared data with existing Hα/Hβ and thermal radio data. For the two OB associations where the mass function has been determined directly, the model correctly "predicts" a solar neighborhood upper mass function within the uncertainties. No evidence is found for upper mass functions significantly different from that in the solar neighborhood.
AB - IRAS far-infrared fluxes are presented for six H II regions in the Large Magellanic Cloud. These regions are the sites of recent, massive star formation where the radiative heating source is young stars rather than the general interstellar radiation field. As such, the observations become building blocks for the interpretation of far-infrared emission from spatially unresolved galaxies. In addition, the multiwavelength luminosities of the region then probe the young stellar upper initial mass function. With the long-range goal of determining the stellar content of unresolved star-forming regions, we present the results of a simple model which combines the infrared data with existing Hα/Hβ and thermal radio data. For the two OB associations where the mass function has been determined directly, the model correctly "predicts" a solar neighborhood upper mass function within the uncertainties. No evidence is found for upper mass functions significantly different from that in the solar neighborhood.
KW - H II regions
KW - Infrared: interstellar: continuum
KW - Magellanic Clouds
KW - Stars: formation
UR - http://www.scopus.com/inward/record.url?scp=11944256025&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=11944256025&partnerID=8YFLogxK
M3 - Article
AN - SCOPUS:11944256025
VL - 397
SP - 542
EP - 551
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 2
ER -