Projects per year
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 |
|---|---|
| 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. (PI), Cameron, A. (CoI), Dominik, M. (CoI), Driver, S. (CoI), Greaves, J. (CoI), Horne, K. (CoI), Jardine, M. (CoI), Wood, K. (CoI) & Zhao, H. (CoI)
Science & Technology Facilities Council
1/04/09 → 31/03/12
Project: Standard