Abstract

view Abstract Citations (128) References (38) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Origin of the Far-Infrared Luminosity from Spiral Galaxies Devereux, Nicholas A. ; Young, Judith S. Abstract The relationship between the far-infrared and Hα luminosity has been investigated for a sample of 124 spiral galaxies. After correcting the Hα luminosities for an average 1 mag of extinction and extrapolating the IRAS 40-120 micron luminosity to 1000 microns, we find that the mean ratio of Hα to far-infrared luminosity is comparable to that expected from H II regions powered by stars with masses > 6 M_sun_. This result constitutes strong evidence in support of the view that high-mass (> 6 M_sun_) O and B stars are responsible for both the Hα and far-infrared emission in spiral galaxies of high, >= 1 x 10^9^ L_sun_, far-infrared luminosity. Publication: The Astrophysical Journal Pub Date: February 1990 DOI: 10.1086/185659 Bibcode: 1990ApJ...350L..25D Keywords: Far Infrared Radiation; H Alpha Line; Interstellar Extinction; Luminosity; Spiral Galaxies; B Stars; H Ii Regions; Stellar Mass; Astrophysics; GALAXIES: STELLAR CONTENT; INFRARED: GENERAL full text sources ADS |

Keywords

PhysicsAstrophysicsLuminositySpiral galaxyLuminous infrared galaxyGalaxyAstronomyExtinction (optical mineralogy)Luminosity functionStarsFar infraredInfraredStellar massStar formation

Related Publications

The mass ratios of Cepheid binaries

view Abstract Citations (52) References (68) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Mass Ratios of Cepheid Binaries Evans, Nancy Re...

1995 The Astrophysical Journal 43 citations

Publication Info

Year
1990
Type
article
Volume
350
Pages
L25-L25
Citations
67
Access
Closed

Social Impact

Social media, news, blog, policy document mentions

Citation Metrics

67
OpenAlex
4
Influential
54
CrossRef

Cite This

Nicholas A. Devereux, Judith S. Young (1990). The origin of the far-infrared luminosity from spiral galaxies. The Astrophysical Journal , 350 , L25-L25. https://doi.org/10.1086/185659

Identifiers

DOI
10.1086/185659

Data Quality

Data completeness: 81%