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1968, A Blaisdell book in the pure and applied sciences, 298
Book
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 07/2019, Volume 879, Issue 1, p. 48
The plane-parallel approximation of the stellar atmospheres cannot be applied to model the formation of optically thick lines formed in extended atmospheres.... 
radiative transfer | SPECTRAL-LINES | COMOVING-FRAME EQUATION | RADIATIVE-TRANSFER | Sun: atmosphere | line: formation | REDISTRIBUTION | line: profiles | ASTRONOMY & ASTROPHYSICS | SYSTEMS | ATOMS | polarization | MAGNETIC-FIELD | FLOWS | RESONANCE LINES | SCATTERING
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2016, Volume 586, p. A156
Journal Article
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2010, Volume 409, Issue 1, pp. 29 - 37
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2015, Volume 452, Issue 2, pp. 1612 - 1612
Line contribution functions are useful diagnostics for studying spectral line formation in stellar atmospheres. I derive an expression for the contribution... 
Stellar atmospheres | Spectral lines | Flux | On-line systems | Mathematical models | Formations | Diagnostic systems | Three dimensional models
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 06/2007, Volume 662, Issue 2, pp. 1148 - 1155
We present detailed NLTE spectral synthesis models of the Type II supernova 2005cs, which occurred in M51 and for which the explosion time is well determined.... 
supernovae : individual (SN 2005cs) | stars : atmospheres | EXPANDING PHOTOSPHERE METHOD | PARALLEL IMPLEMENTATION | LOW-DENSITY PHOTOSPHERES | NON-LTE | PRELIMINARY SPECTRAL-ANALYSIS | IA SUPERNOVA SPECTRA | ASTRONOMY & ASTROPHYSICS | STELLAR ATMOSPHERE PROGRAM | SN 1987A | LARGE-MAGELLANIC-CLOUD | stars : abundances | II-P SUPERNOVAE
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 10/2003, Volume 409, Issue 2, pp. L1 - L4
Rate coefficients for inelastic collisions between Li and H atoms covering all transitions between the asymptotic states Li(2s,2p,3s,3p,3d,4s,4p,4d,4f)+H(1s)... 
RECOMBINATION | AB-INITIO | SPECTRAL-LINES | line : formation | COOL STARS | CURVES | ATOM COLLISIONS | HYDROGEN | atomic data | ASTRONOMY & ASTROPHYSICS | MODEL ATMOSPHERES | MUTUAL NEUTRALIZATION | LITHIUM | stars : abundances
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 04/2011, Volume 731, Issue 2, pp. 114 - jQuery1323909351864='48'
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 09/2011, Volume 739, Issue 1, p. 40
To explain the linear polarization observed in spatially resolved structures in the solar atmosphere, the solution of polarized radiative transfer (RT)... 
Sun: atmosphere | polarization | line: formation | magnetic fields | scattering | radiative transfer | RESONANCE RADIATION | NUMERICAL-METHODS | MATRIX | MAGNETIC-FIELDS | SPECTRAL-LINES | ASTRONOMY & ASTROPHYSICS | RADIATION-FIELD LIMIT | ABSENCE | IRREDUCIBLE COMPONENTS | STOKES PARAMETERS | Physics - Solar and Stellar Astrophysics
Journal Article
Journal of Quantitative Spectroscopy and Radiative Transfer, ISSN 0022-4073, 01/2013, Volume 115, pp. 46 - 59
An expression for the partial frequency redistribution (PRD) matrix for line scattering in a two-term atom, which includes the -state interference between its... 
Polarization | Magnetic fields | Atomic processes | Scattering | Sun atmosphere | Line profiles | RESONANCE RADIATION | MATRIX | SPECTRAL-LINES | CLASSICAL-THEORY | DEPOLARIZATION | SPECTROSCOPY | REGIME | 4227 ANGSTROM LINE | HANLE | Corticosteroids | Physics - Solar and Stellar Astrophysics
Journal Article
2017, ISBN 9789814699075, xvi, 347 pages
"The book presents an advanced tool for experimentalists using spectral lineshapes for diagnostics of laboratory or astrophysical plasmas, and for theorists... 
Plasma astrophysics | Spectral line formation | Plasma diagnostics | Plasma spectroscopy
Book
Journal of Physics: Conference Series, ISSN 1742-6588, 2012, Volume 397, Issue 1, pp. 12018 - 7
An extension of the radiative transfer theory is presented and applied to the formation of spectral lines in optically thick media. In the model, the radiation... 
Mean free path | Spectral lines | Mathematical models | Photons | Formations | Radiative transfer | Plasmas | Formalism
Conference Proceeding
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 10/2019, Volume 631, p. A80
Manganese (Mn) is a key Fe-group element, commonly employed in stellar population and nucleosynthesis studies to explore the role of SN Ia. We have developed a... 
stars: atmospheres | CROSS-SECTIONS | Sun: abundances | STELLAR GRANULATION | LAMBDA ITERATION METHOD | radiative transfer | SPECTRAL-LINES | stars: abundances | MULTILEVEL RADIATIVE-TRANSFER | SAMPLING MODEL ATMOSPHERES | Sun: atmosphere | A-STAR | line: formation | ABUNDANCE ANALYSIS | ASTRONOMY & ASTROPHYSICS | SOLAR | MAFAGS-OS
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 01/2013, Volume 549, pp. 1 - 16
We Investigate the role of convection In the formation of atomic and molecular lines in the atmosphere of a red giant star. For this purpose we study the... 
Red giant stars | Stellar atmospheres | Spectral lines | Silicon | Formations | Carbon monoxide | Three dimensional models | Astronomy
Journal Article
Astrophysics, ISSN 0571-7256, 9/2015, Volume 58, Issue 3, pp. 406 - 419
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 05/2005, Volume 624, Issue 2 I, pp. 1025 - 1037
Within the framework of the quantum theory of polarized line formation, in the limit of complete frequency redistribution and of the collisionless regime, we... 
Polarization | Atomic processes | Line: profiles | Sun: magnetic fields | PARTIAL REDISTRIBUTION | STATES | atomic processes | line : profiles | SPECTRAL-LINES | RESONANCE POLARIZATION | LIMIT | SUN | RADIATION | Sun : magnetic fields | ASTRONOMY & ASTROPHYSICS | SCATTERING POLARIZATION | COLLISIONLESS REGIME | polarization | NAI D-2
Journal Article
Astrophysical Journal, ISSN 0004-637X, 06/2014, Volume 788, Issue 1, pp. 48 - 13
Journal Article
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