Results 321 to 330 of about 882,024 (358)
A binary merger product as the direct progenitor of a Type II-P supernova
Niu* Z +17 more
europepmc +1 more source
Extreme energy in a relaxed galaxy group indicates the bursty nature of AGN feedback
Eckert D +21 more
europepmc +1 more source
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2002
We give an overview about the state-of-the-art in cool stellar (and sub-stellar) atmosphere simulations. Recent developments in numerical methods and parallel supercomputers, as well as in the quality of input data such as atomic and molecular line lists have led to substantial improvements in the quality of synthetic spectra when compared to multi ...
Peter H. Hauschildt +5 more
openaire +1 more source
We give an overview about the state-of-the-art in cool stellar (and sub-stellar) atmosphere simulations. Recent developments in numerical methods and parallel supercomputers, as well as in the quality of input data such as atomic and molecular line lists have led to substantial improvements in the quality of synthetic spectra when compared to multi ...
Peter H. Hauschildt +5 more
openaire +1 more source
Nature, 1971
Stellar Atmospheres . By Dimitri Mihalas. (Series of Books in Astronomy and Astrophysics.) Pp. xiv + 463. (Freeman: San Francisco and Reading, February 1971.) £7.50.
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Stellar Atmospheres . By Dimitri Mihalas. (Series of Books in Astronomy and Astrophysics.) Pp. xiv + 463. (Freeman: San Francisco and Reading, February 1971.) £7.50.
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Do Intrinsic Magnetic Fields Protect Planetary Atmospheres from Stellar Winds?
Space Science Reviews, 2021R. Ramstad, S. Barabash
semanticscholar +1 more source
2004
In this note, the formalism used to compute a simple stellar atmosphere model is described. The definition of a stellar atmosphere is strongly connected with the radiation field crossing the boundary layers of a star: the atmosphere is composed of those layers where photons interact with matter for the last time before leaving the star.
openaire +1 more source
In this note, the formalism used to compute a simple stellar atmosphere model is described. The definition of a stellar atmosphere is strongly connected with the radiation field crossing the boundary layers of a star: the atmosphere is composed of those layers where photons interact with matter for the last time before leaving the star.
openaire +1 more source

