The DOI matches its Crossref record; 8 of the 8 references it cites were found in a registry or an index.
The photospheric barium spectrum: Solar abundance and collision broadening of Baii lines by hydrogen
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Citations
Cites
Meteorites and the Early Solar System
Anders, E. (1971) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.09.090171.000245 · Cited by 1,583
The Harvard-Smithsonian reference atmosphere
Gingerich, O., Noyes, R. W., Kalkofen, W., & Cuny, Y. (1971) · Solar Physics · doi:10.1007/bf00149057 · Cited by 629
Unsöld, A., & Beiser, A. (1956) · Physics Today · doi:10.1063/1.3059998 · Cited by 461
Handbook of elemental abundances in meteorites
Mason, B. H. (1971) · Cited by 357
The Abundances of the Elements in the Solar Atmosphere.
Goldberg, L., Muller, E. A., & Aller, L. H. (1960) · The Astrophysical Journal Supplement Series · doi:10.1086/190053 · Cited by 256
Oscillator Strengths of Ca II, Sr II, and Ba II
Gallagher, A. (1967) · Physical Review · doi:10.1103/physrev.157.24 · Cited by 217
Determinations of concentrations of heavy elements in meteorites by activation analysis
Reed, G. W., Kigoshi, K., & Turkevich, A. (1960) · Geochimica et Cosmochimica Acta · doi:10.1016/0016-7037(60)90055-7 · Cited by 208
Labs, D., & Neckel, H. (1970) · Solar Physics · doi:10.1007/bf00149474 · Cited by 143
Cited by
The Chemical Composition of the Sun
Asplund, M., Grevesse, N., Sauval, A. J., & Scott, P. (2009) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.46.060407.145222 · Cited by 9,346
“The first uncertainty has been estimated by taking half the difference between the results with the spatially-averaged 3D model (denoted <3D>) and the Holweger & Müller (1974) model.”
BackgroundMethodResultInfluentialA grid of MARCS model atmospheres for late-type stars: I. Methods and general properties
Gustafsson, B., Edvardsson, B., Eriksson, K., Jørgensen, U. G., Nordlund, Å., & Plez, B. (2008) · Astronomy & Astrophysics · doi:10.1051/0004-6361:200809724 · Cited by 2,654
ABUNDANCE RATIOS AND GALACTIC CHEMICAL EVOLUTION
McWilliam, A. (1997) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.35.1.503 · Cited by 697
Line formation in solar granulation: IV. [O I], OI and OH lines and the photospheric O abundance
Asplund, M., Grevesse, N., Sauval, A. J., Prieto, C. A., & Kiselman, D. (2003) · arXiv (Cornell University) · doi:10.48550/arxiv.astro-ph/0312290 · Cited by 522
The Galactic Thick Disk Stellar Abundances
Prochaska, J. X., Naumov, S. O., Carney, B. W., McWilliam, A., & Wolfe, A. M. (2000) · The Astronomical Journal · doi:10.1086/316818 · Cited by 422
Metadata
- Authors
- Holweger, H., & M�ller, E. A.
- Venue
- Solar Physics
- Published
- 1974-11
- Volume
- 39
- Issue
- 1
- Pages
- 19-30
- ISSN
- 0038-0938 (ISSN-L)
- 1573-093X
- OpenAlex
- W2106648118
- Cited by
- 585
- References
- 8
- FWCI
- 9.17
- Type
- journal article
- Language
- en
- Open access
- closed
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- CoChat. (2026). Citation check: The photospheric barium spectrum: Solar abundance and collision broadening of Baii lines by hydrogen. https://app.cochat.ai/papers/10.1007/bf00154968
- The paper
- Holweger, H., & M�ller, E. A. (1974). The photospheric barium spectrum: Solar abundance and collision broadening of Baii lines by hydrogen. Solar Physics. https://doi.org/10.1007/bf00154968
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.
