The z ~ 1.5 Tully-Fisher relation

Details The z ~ 1.5 Tully-Fisher relation The z ~ 1.5 Tully-Fisher relation

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005assl..329p..81v&link_type=abstract

Starbursts: From 30 Doradus to Lyman Break Galaxies, Held in Cambridge, UK, 6-10 September 2004. Edited by R. de Grijs and R.M.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We investigate the z˜1.5 rest-frame B-band Tully-Fisher relation, using a sample of Hα-emitting galaxies and find a ˜ 2 mag offset from the local Tully-Fisher relation. We demonstrate why the interpretation of this result is not straightforward: analysis of high-redshift Tully-Fisher relations is plagued by selection effects, biases, observational challenges, and other effects.

Affiliated with

Also associated with

No associations

Rating

The z ~ 1.5 Tully-Fisher relation 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 The z ~ 1.5 Tully-Fisher relation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The z ~ 1.5 Tully-Fisher relation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-768206