Results 121 to 130 of about 146,288 (166)

Mind the Gap. II. The Near-UV Fluxes of M Dwarfs

The Astronomical Journal
Because of the continuous variations in mass, metallicity, and opacity, dwarf stars are distributed along the main sequence on optical and near-IR color–magnitude diagrams following a smooth polynomial.
Wei-Chun Jao, Allison Youngblood
doaj   +1 more source

Astrospheres and Solar-like Stellar Winds. [PDF]

Living Rev Sol Phys, 2004
Wood BE.
europepmc   +1 more source

Beam electrons as a source of Hα flare ribbons. [PDF]

Nat Commun, 2017
Druett M, Scullion E, Zharkova V, Matthews S, Zharkov S, Rouppe Van der Voort L.   +5 more
europepmc   +1 more source

On Methods and Applications in Spectrophotometry. [PDF]

Proc Natl Acad Sci U S A, 1928
Payne CH, Hogg FS.
europepmc   +1 more source

Magnetic activity and spectral behavior of RS CVn binary system (IM Pegasi) in the ultraviolet. [PDF]

Sci Rep
Sanad MR, Rahman HIA, Badawy WA.
europepmc   +1 more source

Intensities of the hydrogen Balmer lines of solar-like stars revealed by the LAMOST spectroscopic surveys. [PDF]

Sci Rep
He H.
europepmc   +1 more source

A Stellar Conversation with scientist, engineer and astronaut Jan Davis

, 2008
Includes descriptive metadata provided by producer in MP3 file: "Stellar Conversations - Podcasts - A Stellar Conversation with scientist, engineer and astronaut Jan Davis." By news@vanderbilt.edu (Vanderbilt News Service).
Chappell, Rick, 1943-, Davis, Jan, 1953-
core  

The Shape of Stellar Convection

Recent space missions such as Kepler, TESS, and soon PLATO have provided an abundance of high-quality stellar data, highlighting the need for more accurate models of stellar structure and evolution.
Mary Geer Dethero
core   +1 more source

Science development study for the Atacama Large Aperture Submillimeter Telescope (AtLAST): Solar and stellar observations. [PDF]

Open Res Eur
Wedemeyer S, Barta M, Brajša R, Chai Y, Costa J, Gary D, Gimenez de Castro G, Gunar S, Fleishman G, Hales A, Hudson H, Kirkaune M, Mohan A, Motorina G, Pellizzoni A, Saberi M, Selhorst CL, Simoes PJA, Shimojo M, Skokić I, Sudar D, Menezes F, White SM, Booth M, Klaassen P, Cicone C, Mroczkowski T, Cordiner MA, Di Mascolo L, Johnstone D, van Kampen E, Lee M, Liu D, Maccarone T, Orlowski-Scherer J, Saintonge A, Smith M, Thelen AE.   +37 more
europepmc   +1 more source

Stellar Chromospheres [PDF]

Annual Review of Astronomy and Astrophysics, 1980
Important progress in our understanding of stellar chromospheres has occurred in the past few years as a result of new observations, developments in spectral line formation theory, and the application of that theory to the construction of detailed model chromospheres.
Linsky, J. L.
exaly   +6 more sources