Results 61 to 70 of about 4,318,459 (158)
, 2002 Study determined if 2MASS photometric data are reliable for luminosity classification using JHK plots of Reid and Hawley (2001). Effects of interstellar reddening on the placement of giant and dwarf data on the JIIK plot were analyzed. Dwarfs (N=54) were
Furiak, Nicolas M.
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Luminosity classification of red stars and distances to nearby red dwarfs
, 2002 This investigation in the 24 Kapteyn Selected Areas along the celestial equator examined 21 red dwarf stars identified in an objective-prism survey.
Maupin, Richard E.
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Continuum and Line Emission of Flares on Red Dwarf Stars: Origin of the Blue Continuum Radiation
, 2016 There are two types of models that explain the appearance of the quasi-blackbody radiation during the impulsive phase of stellar flares. Grinin and Sobolev [Astrophysics, Vol. 13, 348 (1977)] argue that the blue component of the optical continuum is formed in "the transition layer between the chromosphere and the photosphere." Katsova et al ...
openaire +2 more sources
Flare star observations with a single-photon counting imaging detector [PDF]
, 1995 At Los Alamos National Laboratory we are developing a new imaging sensor which combines high spatial and high temporal resolution over a large area format, while maintaining single-photon counting sensitivity and substaining a high count rate.
Baron, M.H. +3 more
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Study of quiescent state X-ray emission from flare stars
, 1986 Quiescent-state X-ray emission of seven flare stars was studied as well as the relationship between the emissions of the chromosphere, transition region and corona.
Rao, A. R. +2 more
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Study of a Non-Solar Star Flare
, 1996 v, 37 p.Violent eruptions on the surfaces of stars, flares are among the most energetic stellar phenomena. They can last anywhere from a few minutes to a few hours, and can emit radiation from long-wavelength radio waves to gamma rays.
Halderson, Eve
core +1 more source
Archival Stellar Flare Follow-up in Evryscope Observations [PDF]
M dwarfs, the most abundant stars in the galaxy, are prime targets in the search for habitable exoplanets. However, their high flare activity may compromise planetary atmospheres, with Coronal Mass Ejections (CMEs) increasing this risk. Despite this, the
Thomas, Tyler J
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White dwarf-red dwarf binaries in the Galaxy [PDF]
, 2007 Contains fulltext : 30919.pdf (Publisher’s version ) (Open Access)This PhD thesis shows several studies on white dwarf - red dwarf binaries.
Besselaar, E.J.M. van den
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Determination of the physical parameters of the eclipsing dwarf nova system IP Peg
, 1998 IP Peg is a member of a family of star systems known as cataclysmic variable stars, CVs. CVs are star systems in which a red dwarf star orbits a white dwarf and mass transfer is taking place from the red dwarf to the white dwarf.
Bryant, Jeffrey M.
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88th Annual Meeting of the Meteoritical Society 2026: Abstracts
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley +1 more source