Pith. sign in

REVIEW

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

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 0908.1904 v1 pith:MYT6TRBF submitted 2009-08-13 astro-ph.GA astro-ph.CO

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

M. Cappellari , N. Scott , K. Alatalo , L. Blitz , M. Bois , F. Bournaud , M. Bureau , R. L. Davies
show 17 more authors
T. A. Davis P. T. de Zeeuw E. Emsellem J. Falcon-Barroso S. Khochfar D. Krajnovic H. Kuntschner P.-Y. Lablanche R. M. McDermid R. Morganti T. Naab M. Sarzi P. Serra R. C. E. van den Bosch G. van de Ven A. Weijmans L. M. Young
This is my paper
classification astro-ph.GA astro-ph.CO
keywords stellarearly-typeetgsgalaxiesrelationsscalingatlas3dconstructing
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
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).

discussion (0)

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