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

Whitaker, Katherine E.; Bezanson, Rachel; van Dokkum, Pieter G.; Franx, Marijn; van der Wel, Arjen; Brammer, Gabriel; Förster-Schreiber, Natascha M.; Giavalisco, Mauro; Labbé, Ivo; Momcheva, Ivelina G.; Nelson, Erica J.; Skelton, Rosalind

doi:10.3847/1538-4357/aa6258

アイテム詳細

登録内容を編集ファイル形式で保存

一時保存へ追加

タグ情報を表示リリース履歴を表示詳細要約

公開

学術論文

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

There are no locators available

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

フルテキスト (公開)

公開されているフルテキストはありません

付随資料 (公開)

There is no public supplementary material available

引用

Whitaker, K. E., Bezanson, R., van Dokkum, P. G., Franx, M., van der Wel, A., Brammer, G., Förster-Schreiber, N. M., Giavalisco, M., Labbé, I., Momcheva, I. G., Nelson, E. J., & Skelton, R. (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):, pp. 1-19. doi:10.3847/1538-4357/aa6258.

引用: https://hdl.handle.net/11858/00-001M-0000-002D-8041-8

要旨

要旨はありません