English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

Predicting quiescence: the dependence of specific star formation rate on galaxy size and central density at 0.5 < z < 2.5

MPS-Authors
/persons/resource/persons4923

Förster-Schreiber,  Natascha M.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons204550

Nelson,  Erica J.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available
Citation

Whitaker, K. E., Bezanson, R., van Dokkum, P. G., Franx, M., van der Wel, A., Brammer, G., et al. (2017). Predicting quiescence: the dependence of specific star formation rate on galaxy size and central density at 0.5 < z < 2.5. The Astrophysical Journal, 838(1): 19, pp. 1-19. doi:10.3847/1538-4357/aa6258.


Cite as: https://hdl.handle.net/11858/00-001M-0000-002D-8041-8
Abstract
There is no abstract available