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Bhatia, A. K., Kastner, S. O. (1993) The Optically Thick C III Spectrum. I. Term Populations and Multiplet Intensities at Lower Optical Depths: Erratum. The Astrophysical Journal, 417. 826pp. doi:10.1086/173363

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Reference TypeJournal (article/letter/editorial)
TitleThe Optically Thick C III Spectrum. I. Term Populations and Multiplet Intensities at Lower Optical Depths: Erratum
JournalThe Astrophysical Journal
AuthorsBhatia, A. K.Author
Kastner, S. O.Author
Year1993 (November)Volume417
PublisherIOP Publishing
DOIdoi:10.1086/173363Search in ResearchGate
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Mindat Ref. ID3333935Long-form Identifiermindat:1:5:3333935:7
GUID0
Full ReferenceBhatia, A. K., Kastner, S. O. (1993) The Optically Thick C III Spectrum. I. Term Populations and Multiplet Intensities at Lower Optical Depths: Erratum. The Astrophysical Journal, 417. 826pp. doi:10.1086/173363
Plain TextBhatia, A. K., Kastner, S. O. (1993) The Optically Thick C III Spectrum. I. Term Populations and Multiplet Intensities at Lower Optical Depths: Erratum. The Astrophysical Journal, 417. 826pp. doi:10.1086/173363
In(1993) The Astrophysical Journal Vol. 417. IOP Publishing

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Bhatia, A. K., Kastner, S. O. (1992) The optically thick C III spectrum. I - Term populations and multiplet intensities at lower optical depths. The Astrophysical Journal Supplement Series, 79. 139 doi:10.1086/191648
Bhatia, A. K., Kastner, S. O. (1993) The optically thick C III spectrum. 2: Level/term populations and line/multiplet intensities using an improved hybrid model. The Astrophysical Journal Supplement Series, 89. 227 doi:10.1086/191846
Bhatia, A. K., Kastner, S. O. (1993) The optically thin C III spectrum - Line and multiplet intensities. The Astrophysical Journal, 408. 744pp. doi:10.1086/172634
Kastner, S. O., Bhatia, A. K. (1997) The Neutral Nitrogen Spectrum: Term Populations, Multiplet Intensities, Diagnostic Diagrams, and Comparisons with Observations. The Astrophysical Journal Supplement Series, 109 (1) 241-267 doi:10.1086/312974
Kastner, S. O., Bhatia, A. K. (1989) The optically thick O III spectrum. I - Diagnostic ratios involving the intercombination lines. The Astrophysical Journal Supplement Series, 71. 665 doi:10.1086/191392
Bhatia, A. K., Kastner, S. O. (1995) The neutral oxygen spectrum. 1: Collisionally excited level populations and line intensities under optically thin conditions. The Astrophysical Journal Supplement Series, 96. 325 doi:10.1086/192121
Kastner, S. O., Bhatia, A. K. (1992) On the calculation of atomic term populations. The Astrophysical Journal, 398. 698pp. doi:10.1086/171894
Bhatia, A. K., Kastner, S. O. (1988) Spatial probing of nebular properties via Bowen pumping. The Astrophysical Journal, 331. 826pp. doi:10.1086/166602
Bhatia, A. K., Kastner, S. O. (1999) The Optically Thick FexviiSpectrum: X‐Ray, Extreme‐Ultraviolet, and Forbidden Line Ratios. The Astrophysical Journal, 516 (1). 482-489 doi:10.1086/307085
Kastner, S. O., Bhatia, A. K. (2001) Optically Thin and Thick FexvSpectrum: Effect of Self‐Absorption on the 284.16 A Resonance Line. The Astrophysical Journal, 553 (1). 421-428 doi:10.1086/320649
Kastner, S. O., Bhatia, A. K. (1993) C III spectra in WC Wolf-Rayet stars - Does collisional excitation dominate?. The Astrophysical Journal, 406. 708pp. doi:10.1086/172481
 
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