The DOI matches its Crossref record.
Soft X-ray spectrum of a hot plasma
Abstract
The spectrum of radiation emitted by a hot optically thin plasma with abundances and equilibrium ionization balance appropriate to interstellar conditions has been calculated. The results at wavelengths shorter than 200 A are discussed for material in the electron-temperature range from 160,000 to 100 million K.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cited by
Starburst‐driven Mass Loss from Dwarf Galaxies: Efficiency and Metal Ejection
Mac Low, M., & Ferrara, A. (1999) · The Astrophysical Journal · doi:10.1086/306832 · Cited by 986
The stellar-activity-rotation relationship and the evolution of stellar dynamos
Wright, N. J., Drake, J. J., Mamajek, E. E., & Henry, G. W. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/743/1/48 · Cited by 882
Chandra X‐Ray Spectroscopic Imaging of Sagittarius A* and the Central Parsec of the Galaxy
Baganoff, F. K., Maeda, Y., Morris, M., Bautz, M. W., Brandt, W. N., Cui, W., Doty, J. P., Feigelson, E. D., Garmire, G. P., Pravdo, S. H., et al. (2003) · The Astrophysical Journal · doi:10.1086/375145 · Cited by 809
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
Pauldrach, A. W. A., Hoffmann, T. L., & Lennon, M. (2001) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20010805 · Cited by 517
Metadata
- Authors
- Raymond, J. C., & Smith, B. W.
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Published
- 1977-12
- Volume
- 35
- Pages
- 419
- ISSN
- 0067-0049 (ISSN-L)
- 1538-4365
- OpenAlex
- W2039720425
- Cited by
- 1,345
- References
- 0
- Type
- conference abstract
- Language
- en
- Open access
- closed
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
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: Soft X-ray spectrum of a hot plasma. https://app.cochat.ai/papers/10.1086/190486
- The paper
- Raymond, J. C., & Smith, B. W. (1977). Soft X-ray spectrum of a hot plasma. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/190486
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
