Intergalactic Medium Contribution
Intergalactic Medium Contribution is a theoretical construct in astrophysics that denotes the specific component of the X-ray background radiation arising from diffuse, hot plasma located in the intergalactic space, distinguished from other sources by its spatial distribution and thermal emission characteristics.
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George B. Field · The Astrophysical Journal · 1965 · 1.4K citations
Natural Sciences, Astronomy, Physics +14
A NEW ELECTRON-DENSITY MODEL FOR ESTIMATION OF PULSAR AND FRB DISTANCES
The Astrophysical Journal · 2017 · 1.1K citations · Full text
Natural Sciences, Astronomy, Physics +14
The Chemical Evolution of the Galaxy: The Two‐Infall Model
C. Chiappini, F. Matteuccí, R. Gratton · The Astrophysical Journal · 1997 · 941 citations · Full text
Natural Sciences, Astronomy, Physics +17
Brant Robertson, Richard S. Ellis, Steven R. Furlanetto et al. · The Astrophysical Journal Letters · 2015 · 895 citations · Full text
Natural Sciences, Astronomy, Physics +17
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University of California, Los Angeles, United States
32 publications · 3.8K citations
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
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California Institute of Technology
Pasadena, United States
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187 publications
19.4K citations
University of California, Santa Cruz
Santa Cruz, United States
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123 publications
15.6K citations
University of Cambridge
Cambridge, United Kingdom
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190 publications
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Max Planck Institute for Astrophysics
Garching, Germany
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Max Planck Institute for Astronomy
Heidelberg, Germany
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163 publications
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Centre National de la Recherche Scientifique
Paris, France
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University of California, Berkeley
Berkeley, United States
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ApJ · 504 publications · 45.6K citations
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