Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter haloes-Reference-Cited by-同舟云学术

Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter haloes

Published:2018-12-18 Issue:4 Volume:483 Page:4922-4937
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Baugh C M¹,Gonzalez-Perez Violeta²^ORCID,Lagos Claudia D P³^ORCID,Lacey Cedric G¹^ORCID,Helly John C¹,Jenkins Adrian¹^ORCID,Frenk Carlos S¹,Benson Andrew J⁴^ORCID,Bower Richard G¹^ORCID,Cole Shaun¹

Affiliation:

1. Institute for Computational Cosmology, Department of Physics, Science Laboratories, Durham University, South Road, Durham DH1 3LE, UK

2. Institute of Cosmology and Gravitation, Portsmouth University, Dennis Sciama Building, Burnaby Road, Portsmouth PO1 3FX, UK

3. International Centre for Radio Astronomy Research, 7 Fairway, Crawley, 6009 Perth, WA, Australia

4. Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101, USA

Funder

Durham University

Science and Technology Facilities Council

British Infection Society

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/483/4/4922/27441217/sty3427.pdf

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