pith. the verified trust layer for science. sign in

arxiv: 0908.1904 · v1 · pith:MYT6TRBFnew · submitted 2009-08-13 · 🌌 astro-ph.GA · astro-ph.CO

Scaling relations in early-type galaxies from integral-field stellar kinematics

classification 🌌 astro-ph.GA astro-ph.CO
keywords stellarearly-typeetgsgalaxiesrelationsscalingatlas3dconstructing
0
0 comments X p. Extension
Add this Pith Number to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{MYT6TRBF}

Prints a linked pith:MYT6TRBF badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

We study the origin of the scaling relations of early-type galaxies (ETGs) by constructing detailed models of the stellar dynamics for the K-band selected, volume-limited ATLAS3D sample of 263 nearby ETGs, spanning a large range of masses and stellar velocity dispersions (60 < sigma < 350 km/s).

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.