Dust attenuation, bulge formation, and inside-out quenching of star formation 
in star-forming main sequence galaxies at z ~ 2

Tacchella, S.; Carollo, C. M.; Förster Schreiber, N. M.; Renzini, A.; Dekel, A.; Genzel, R.; Lang, P.; Lilly, S. J.; Mancini, C.; Onodera, M.; Tacconi, L. J.; Wuyts, S.; Zamorani, G.

doi:10.3847/1538-4357/aabf8b

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

Dust attenuation, bulge formation, and inside-out quenching of star formation in star-forming main sequence galaxies at z ~ 2

MPS-Authors

/persons/resource/persons4923

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

/persons/resource/persons4590

Genzel, R.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons132103

Lang, P.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4582

Tacconi, L. 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

Tacchella, S., Carollo, C. M., Förster Schreiber, N. M., Renzini, A., Dekel, A., Genzel, R., et al. (2018). Dust attenuation, bulge formation, and inside-out quenching of star formation in star-forming main sequence galaxies at z ~ 2. The Astrophysical Journal, 859(1): 56. doi:10.3847/1538-4357/aabf8b.

Cite as: https://hdl.handle.net/21.11116/0000-0002-4B96-1

Abstract

There is no abstract available