Stellar mass dependence of evolution of color and morphology of galaxies in HDF-N

Details Stellar mass dependence of evolution of color and morphology of galaxies in HDF-N Stellar mass dependence of evolution of color and morphology of galaxies in HDF-N

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005asthe..98..518k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 98, No. 8, p. 518 - 524 (2005)

Astronomy and Astrophysics

Astronomy

Galaxies: Stellar Masses

Scientific paper

Using very deep Subaru K'-band imaging and archival Hubble Space Telescope data of the HDF-N, we investigate the evolution of stellar mass, color and morphology of galaxies to z~3. We mainly examined the rest-frame U-V color distribution of galaxies as a function of stellar mass, and found that galaxies with stellar mass smaller than ~5×109 Msolar are likely to have a relatively long star formation timescale, while the star formation seems to be suppressed in more massiv galaxies at 0

Affiliated with

Also associated with

No associations

Rating

Stellar mass dependence of evolution of color and morphology of galaxies in HDF-N does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Stellar mass dependence of evolution of color and morphology of galaxies in HDF-N, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar mass dependence of evolution of color and morphology of galaxies in HDF-N will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1347706