Sub-eddington Accretion
Sub-Eddington Accretion is an accretion process in which the mass inflow rate onto a compact object remains below the Eddington limit, thereby allowing stable radiative efficiency and preventing radiation pressure from halting further infall.
114
Publications
13.5K
Citations
263
Authors
207
Institutions
Publications per year
2017–2026
35
Parents
114
M. A. Abramowicz, B. Czerny, J. P. Lasota et al. · The Astrophysical Journal · 1988 · 1.6K citations
Natural Sciences, Astronomy, Physics +15
Black Holes, Galaxy Formation, and the <i>M</i> <sub>BH</sub> - Relation
A. R. King · The Astrophysical Journal · 2003 · 808 citations · Full text
Natural Sciences, Astronomy, Physics +13
A scheme to unify low-power accreting black holes
H. Falcke, Elmar Körding, Sera Markoff · Astronomy and Astrophysics · 2004 · 771 citations · Full text
Natural Sciences, Astronomy, Physics +15
1–5 of 114
263
6
h-index
6
h-index
6
h-index
5
h-index
5
h-index
1–5 of 263
207
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
14 h-index
27 publications
3.5K citations

Centre National de la Recherche Scientifique
Paris, France
11 h-index
25 publications
1.7K citations
Institut d'Astrophysique de Paris
Paris, France
9 h-index
13 publications
753 citations
Goddard Space Flight Center
Greenbelt, United States
9 h-index
13 publications
816 citations
University of Cambridge
Cambridge, United Kingdom
7 h-index
13 publications
489 citations

Sorbonne Université
Paris, France
7 h-index
11 publications
599 citations

Radboud University Nijmegen
Nijmegen, The Netherlands
7 h-index
7 publications
1.7K citations
University of Southampton
Southampton, United Kingdom
7 h-index
13 publications
680 citations
1–8 of 207
39 publications · 4.4K citations
29
h-index
ApJ · 38 publications · 5.2K citations
28
h-index
11 publications · 1.5K citations
11
h-index
7 publications · 806 citations
7
h-index
4 publications · 290 citations
4
h-index
1–5