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Interstellar photoelectric absorption cross sections, 0.03-10 keV
Abstract
An effective absorption cross section per hydrogen atom has been calculated as a function of energy in the 0.03-10 keV range using the most recent atomic cross section and cosmic abundance data. Coefficients of a piecewise polynomial fit to the numerical results are given to allow convenient application in automated calculations.
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Cited by
Buchner, J., Georgakakis, A., Nandra, K., Hsu, L., Rangel, C., Brightman, M., Merloni, A., Salvato, M., Donley, J., & Kocevski, D. (2014) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201322971 · Cited by 1,644
Esin, A. A., McClintock, J. E., & Narayan, R. (1997) · The Astrophysical Journal · doi:10.1086/304829 · Cited by 1,313
ROSAT Survey Diffuse X‐Ray Background Maps. II.
Snowden, S. L., Egger, R., Freyberg, M. J., McCammon, D., Plucinsky, P. P., Sanders, W. T., Schmitt, J. H. M. M., Trumper, J., & Voges, W. (1997) · The Astrophysical Journal · doi:10.1086/304399 · Cited by 602
Self-citationThe Evolution of Compact Binary Star Systems
Postnov, K. A., & Yungelson, L. R. (2014) · Living Reviews in Relativity · doi:10.12942/lrr-2014-3 · Cited by 486
Second ROSAT all-sky survey (2RXS) source catalogue
Boller, T., Freyberg, M. J., Trümper, J., Haberl, F., Voges, W., & Nandra, K. (2016) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201525648 · Cited by 486
Metadata
- Authors
- Morrison, R., & McCammon, D.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1983-07
- Volume
- 270
- Pages
- 119
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2017396100
- Cited by
- 1,744
- References
- 0
- FWCI
- 4.74
- Type
- journal article
- Language
- en
- Open access
- closed
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- Morrison, R., & McCammon, D. (1983). Interstellar photoelectric absorption cross sections, 0.03-10 keV. The Astrophysical Journal. https://doi.org/10.1086/161102
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Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.