Origin and Evolution of X-Ray Binaries and Binary Radio Pulsars
Abstract
My life has been an interesting voyage. I became an astronomer because I could not imagine living on Earth and not trying to understand how the Universe works. My scientific career has revolved around observing the motions of stars within galaxies and the ...Read More
Integrity signals
Registry
Cites
Statistics
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
A black hole would likely be a much stronger source of X-rays (L_X > 10^32 erg s^-1) than observed (L_X about 10^30 erg s^-1) if it accreted from a disk.
“A black hole would likely be a much stronger source of X-rays (L X > 10 32 erg s -1 ; Verbunt 1993) than observed (L X 10 30 erg s -1 ) if it accreted from a disk.”
Cited by
Sorted by citations
Mamajek, E. E., Quillen, A. C., Pecaut, M. J., Moolekamp, F., Scott, E. L., Kenworthy, M. A., Cameron, A. C., & Parley, N. R. (2012) · The Astronomical Journal · doi:10.1088/0004-6256/143/3/72 · Cited by 140 · see citing works
“A black hole would likely be a much stronger source of X-rays (LX > 10 32 erg s−1; Verbunt 1993) than observed (LX ≃ 10 30 erg s−1) if it accreted from a disk.”
Background
- Authors
- Verbunt, F.
- Corresponding author
- Verbunt, Frank
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 1993-09
- Volume
- 31
- Issue
- 1
- Pages
- 93-127
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2178750233
- Cited by
- 202
- References
- 0
- Citations by year
- 2026: 5 · 2025: 12 · 2024: 10 · 2023: 11 · 2022: 11 · 2021: 4 · 2020: 5 · 2019: 4 · 2018: 4 · 2017: 9 · 2016: 9 · 2015: 5 · 2014: 5 · 2013: 9 · 2012: 3
- FWCI
- 9.01
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Annual Review of Astronomy and Astrophysics (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Gamma-ray bursts and supernovae
- Keywords
- X-ray binaries, binary pulsars, binary star evolution, neutron stars, stellar evolution, binary star dynamics
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
