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The top documents tagged [balmer lines]
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balmer lines
Stellar Spectra AST 112 Lecture 7. Stellar Spectra The interior of a star can be considered a “hot dense object” that emits a continuous spectrum. The.
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The planetary nebula M2-9: Balmer line profiles of the nuclear region Silvia Torres-Peimbert 1 Anabel Arrieta 2 Leonid Georgiev 1 1 Instituto de Astronomía,
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Qingkang Li Department of Astronomy Beijing Normal University The Third Workshop of SONG, April, 2010 Disks of Be Stars & Their Pulsations &
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John T. McGraw, Professor Laurel Ladwig, Planetarium Manager
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CSI661/ASTR530 Spring, 2009 Chap. 2 An Overview of Stellar Evolution Jan 28, 2009 Jie Zhang Copyright ©
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Non-LTE studies of A-type supergiants
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Evolutionary Population Synthesis models Divakara Mayya INAOEydm Advanced Lectures on Galaxies (2008 INAOE): Chapter 4.
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Black Hole Masses from Reverberation Mapping
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The Size, Structure & Ionization of the Broad-Line Region in NGC 3227 and NGC 4051
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Non-LTE studies of A-type supergiants Norbert Przybilla K. Butler (Munich), M. Firnstein & F. Schiller (ex-Bamberg)
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FUors : the smoking gun for episodic accretion, or misfit young stars?
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Cosmic Perspective Sec. 15.1
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