GAMA/H-ATLAS: the dust opacity-stellar mass surface density relation for spiral galaxies

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

Gespeichert in:

Bibliographische Detailangaben
Hauptverfasser:	Grootes, MW, Tuffs, RJ, Popescu, CC, Pastrav, B, Andrae, E, Gunawardhana, M, Kelvin, LS, Liske, J, Seibert, M, Taylor, EN, Graham, AW, Baes, Maarten, Baldry, IK, Bourne, N, Brough, S, Cooray, A, Dariush, A, De Zotti, G, Driver, SP, Dunne, L, Gomez, H, Hopkins, AM, Hopwood, R, Jarvis, M, Loveday, J, Maddox, S, Madore, BF, Michalowski, Michal, Norberg, P, Parkinson, HR, Prescott, M, Robotham, ASG, Smith, DJB, Thomas, D, Valiante, E
Format:	Artikel
Sprache:	eng
Schlagworte:	dust extinction galaxies: fundamental parameters galaxies: ISM galaxies: spiral Physics and Astronomy
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Beschreibung
Zusammenfassung:	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
ISSN:	0004-637X