The low-mass end of the baryonic Tully–Fisher relation-Reference-Cited by-同舟云学术

The low-mass end of the baryonic Tully–Fisher relation

Published:2016-09-28 Issue:2 Volume:464 Page:2419-2428
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Sales Laura V.,Navarro Julio F.,Oman Kyle,Fattahi Azadeh,Ferrero Ismael,Abadi Mario,Bower Richard,Crain Robert A.,Frenk Carlos S.,Sawala Till,Schaller Matthieu,Schaye Joop,Theuns Tom,White Simon D. M

Funder

Science and Technology Facilities Council

ERC

BIS

STFC

European Research Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/464/2/2419/18517613/stw2461.pdf

Reference74 articles.

1. Simulations of Galaxy Formation in a Λ Cold Dark Matter Universe. I. Dynamical and Photometric Properties of a Simulated Disk Galaxy

2. DWARF GALAXY DARK MATTER DENSITY PROFILES INFERRED FROM STELLAR AND GAS KINEMATICS

3. Towards a more realistic population of bright spiral galaxies in cosmological simulations

4. Baryonic TullyâFisher relation for extremely low mass Galaxies

5. Stellar Mass‐to‐Light Ratios and the Tully‐Fisher Relation

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