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Abstract
We report the discovery of a well-defined correlation between B-band face-on central optical depth due to dust, tau(f)(B), and the stellar mass surface density, mu(*), of nearby (z
Original language | English |
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Article number | 59 |
Number of pages | 17 |
Journal | Astrophysical Journal |
Volume | 766 |
Issue number | 1 |
DOIs | |
Publication status | Published - 20 Mar 2013 |
Keywords
- dust, extinction
- galaxies: fundamental parameters
- galaxies: ISM
- galaxies: spiral
- SPECTRAL ENERGY-DISTRIBUTION
- STAR-FORMING GALAXIES
- DIGITAL-SKY-SURVEY
- SCIENCE DEMONSTRATION PHASE
- ASSEMBLY GAMA
- HERSCHEL-ATLAS
- METALLICITY RELATION
- RADIATIVE-TRANSFER
- INTERSTELLAR-MEDIUM
- SOLAR NEIGHBORHOOD
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Dive into the research topics of 'GAMA/H-ATLAS: THE DUST OPACITY-STELLAR MASS SURFACE DENSITY RELATION FOR SPIRAL GALAXIES'. Together they form a unique fingerprint.Projects
- 1 Finished
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Astrophysics in St Andrews: Astrophysics in St Andrews / SUPA (Continuan of Rolling Grant - XPP089
Bonnell, I. A. (PI), Cameron, A. C. (CoI), Dominik, M. (CoI), Driver, S. P. (CoI), Greaves, J. S. (CoI), Horne, K. D. (CoI), Jardine, M. M. (CoI), Wood, K. (CoI) & Zhao, H. (CoI)
Science & Technology Facilities Council
1/04/09 → 31/03/12
Project: Standard