Mahalo-subaru: Mapping star formation at the peak epoch of massive galaxy formation

14Citations
Citations of this article
10Readers
Mendeley users who have this article in their library.

Abstract

MAHALO-Subaru (MApping HAlpha and Lines of Oxygen with Subaru) is our on-going large programme which aims to investigate how the star forming activities in galaxies are propagated as a function of time, mass, and environment. We are targeting 10 clusters and proto-clusters at 0.4 2, which suggests that the mode of star formation and/or the activation of AGN are dependent on environment, and thus holding the key to the environmental effects at the early stage of cluster galaxies formation and evolution. © 2013 International Astronomical Union.

Cite

CITATION STYLE

APA

Kodama, T., Hayashi, M., Koyama, Y., Tadaki, K. I., Tanaka, I., & Shimakawa, R. (2012). Mahalo-subaru: Mapping star formation at the peak epoch of massive galaxy formation. In Proceedings of the International Astronomical Union (Vol. 8, pp. 74–77). https://doi.org/10.1017/S1743921313004353

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free