Revealing the Ionization Properties of the Magellanic Stream Using Optical Emission-Reference-Cited by-同舟云学术

Revealing the Ionization Properties of the Magellanic Stream Using Optical Emission

Published:2017-12-18 Issue:2 Volume:851 Page:110
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Barger K. A.^ORCID,Madsen G. J.,Fox A. J.^ORCID,Wakker B. P.^ORCID,Bland-Hawthorn J.^ORCID,Nidever D.^ORCID,Haffner L. M.^ORCID,Antwi-Danso Jacqueline,Hernandez Michael,Lehner N.^ORCID,Hill A. S.^ORCID,Curzons A.,Tepper-García T.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/851/i=2/a=110/pdf

Reference103 articles.

1. THE SPECTRUM AND MORPHOLOGY OF THEFERMIBUBBLES

2. The Chemical Composition of the Sun

3. WARM IONIZED GAS REVEALED IN THE MAGELLANIC BRIDGE TIDAL REMNANT: CONSTRAINING THE BARYON CONTENT AND THE ESCAPING IONIZING PHOTONS AROUND DWARF GALAXIES

4. PRESENT-DAY GALACTIC EVOLUTION: LOW-METALLICITY, WARM, IONIZED GAS INFLOW ASSOCIATED WITH HIGH-VELOCITY CLOUD COMPLEX A

5. Are the Magellanic Clouds on Their First Passage about the Milky Way?

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