The DOI matches its Crossref record; 16 of the 16 references it cites were found in a registry or an index.
The NextGen Model Atmosphere Grid for \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $3000\leq T_{\mathrm{eff}\,}\leq \mathrm{10,000}\,$ \end{document} K
Open accessAbstract
We present our NextGen Model Atmosphere grid for low-mass stars for effective temperatures larger than 3000 K. These LTE models are calculated with the same basic model assumptions and input physics as the VLMS part of the NextGen grid so that the complete grid can be used, e.g., for consistent stellar evolution calculations and for internally consistent analysis of cool star spectra. This grid is also the starting point for a large grid of detailed NLTE model atmospheres for dwarfs and giants. The models were calculated from 3000 to 10,000 K (in steps of 200 K) for 3.5 ≤ log g ≤ 5.5 (in steps of 0.5) and metallicities of -4.0 ≤ [M/H] ≤ 0.0. We discuss the results of the model calculations and compare our results to the Kurucz grid. Some comparisons to standard stars like Vega and the Sun are presented and compared with detailed NLTE calculations.
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Cites
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The HITRAN molecular database: Editions of 1991 and 1992
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Partridge, H., & Schwenke, D. W. (1997) · The Journal of Chemical Physics · doi:10.1063/1.473987 · Cited by 1,155
Model atmospheres for M (sub)dwarf stars. 1: The base model grid
Allard, F., & Hauschildt, P. H. (1995) · The Astrophysical Journal · doi:10.1086/175708 · Cited by 424
Self-citationParallel Implementation of the PHOENIX Generalized Stellar Atmosphere Program
Hauschildt, P. H., Baron, E., & Allard, F. C. (1997) · The Astrophysical Journal · doi:10.1086/304233 · Cited by 272
Self-citationSpectroscopic Properties of the H 3 + Molecule: A New Calculated Line List
Neale, L., Miller, S., & Tennyson, J. (1996) · The Astrophysical Journal · doi:10.1086/177341 · Cited by 210
The Behavior of Chemical Elements in Stars
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Measurements of the Curves-of-Growth of Hot Water Vapor
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Cited by
MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
Choi, J., Dotter, A., Conroy, C., Cantiello, M., Paxton, B., & Johnson, B. D. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/823/2/102 · Cited by 2,922
INTRINSIC COLORS, TEMPERATURES, AND BOLOMETRIC CORRECTIONS OF PRE-MAIN-SEQUENCE STARS
Pecaut, M. J., & Mamajek, E. E. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/208/1/9 · Cited by 2,407
The Limiting Effects of Dust in Brown Dwarf Model Atmospheres
Allard, F., Hauschildt, P. H., Alexander, D. R., Tamanai, A., & Schweitzer, A. (2001) · The Astrophysical Journal · doi:10.1086/321547 · Cited by 1,062
Self-citationModels of very-low-mass stars, brown dwarfs and exoplanets
Allard, F., Homeier, D., & Freytag, B. (2012) · Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences · doi:10.1098/rsta.2011.0269 · Cited by 921
Self-citationTHE OCCURRENCE RATE OF SMALL PLANETS AROUND SMALL STARS
Dressing, C. D., & Charbonneau, D. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/767/1/95 · Cited by 749
Metadata
- Authors
- Hauschildt, P. H., Allard, F., & Baron, E.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1999-02-10
- Volume
- 512
- Issue
- 1
- Pages
- 377-385
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W4292406868
- Cited by
- 1,207
- References
- 16
- FWCI
- 28.14
- Type
- journal article
- Language
- en
- Open access
- bronze
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- CoChat. (2026). Citation check: The NextGen Model Atmosphere Grid for \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $3000\leq T_{\mathrm{eff}\,}\leq \mathrm{10,000}\,$ \end{document} K. https://app.cochat.ai/papers/10.1086/306745
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- Hauschildt, P. H., Allard, F., & Baron, E. (1999). The NextGen Model Atmosphere Grid for \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $3000\leq T_{\mathrm{eff}\,}\leq \mathrm{10,000}\,$ \end{document} K. The Astrophysical Journal. https://doi.org/10.1086/306745
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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.
