The evolution of structure and feedback with Arcus-Reference-Cited by-同舟云学术

The evolution of structure and feedback with Arcus

Published:2016-07-18 Issue: Volume: Page:
ISSN:0277-786X
Container-title:SPIE Proceedings
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Author:

Brenneman Laura W.¹,Smith Randall K.¹,Bregman J.²,Kaastra J.³,Brickhouse N.¹,Allured R.¹,Foster A.¹,Wolk S.¹,Wilms J.⁴,Valencic L.⁵,Willingale R.⁶,Grant C.⁷,Bautz M.⁷,Heilmann R.⁷,Huenemoerder D.⁷,Miller E.⁷,Nowak M.⁷,Schattenburg M.⁷,Schulz N.⁷,Burwitz V.⁸,Nandra K.⁸,Sanders J.⁸,Bookbinder J.⁹,Petre R.⁴,Ptak A.⁴,Smale A.⁴,Burrows D.¹⁰,Poppenhaeger K.¹¹,Costantini E.³,DeRoo C.¹²,McEntaffer R.¹²,Mushotzky R.¹³,Miller J. M.²,Temi P.⁹

Affiliation:

1. Smithsonian Astrophysical Observatory (United States)

2. Univ. of Michigan (United States)

3. SRON (Netherlands)

4. Astronomisches Institut der Univ. Erlangen-Nürnberg (Germany)

5. Johns Hopkins Univ. (United States)

6. Univ. of Leicester (United Kingdom)

7. Massachusetts Institute of Technology (United States)

8. Max-Planck-Institut für extraterrestrische Physik (Germany)

9. NASA Ames Research Ctr. (United States)

10. Pennsylvania State Univ. (United States)

11. Queen's Univ. Belfast (United Kingdom)

12. The Univ. of Iowa (United States)

13. Univ. of Maryland, College Park (United States)

Publisher

SPIE

Reference78 articles.

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3. THE NATURE OF THE WARM/HOT INTERGALACTIC MEDIUM. I. NUMERICAL METHODS, CONVERGENCE, AND O VI ABSORPTION

4. COINCIDENCES BETWEEN O VI AND O VII LINES: INSIGHTS FROM HIGH-RESOLUTION SIMULATIONS OF THE WARM-HOT INTERGALACTIC MEDIUM

5. Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation

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