Suggested Topics within your search.
Suggested Topics within your search.
Cameras
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Electromagnetic wave emission
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Far ultraviolet
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Galaxies: star formation
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Giant stars
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Globular cluster: individual: m30 (NGC 7099)
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H ii region
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Methods. Data analysis
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Physical properties
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Stars
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Stars: horizontal branch
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Stellars
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Techniques: photometric
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Ultraviolet: stars
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galaxies: star formation
1
globular clusters: individual: M30 (NGC 7099)
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methods: data analysis
1
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1Extra-solar planetary atmospheres and interior structure : implications for observational signaturesby Bending, Victoria Louise“... the same face to the star, these gas giants are bathed in intense irradiation, and inhabit a regime alien...”
Published 2016
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2by T. V. Mishenina“... giants, R stars, Li-strong giants, SMR stars have been discussed....”
Published 2017-09-01
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3by Dimitri Veras“... processes which affect planets, asteroids, comets and pebbles as their parent stars evolve into giant branch...”
Published 2016-01-01
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4“... in sunspot spectra, SC-stars, cool M-giant stars and other prominent astrophysical sources....”
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5by Casanellas Jordi“... models. To conclude, we discuss the prospects to use CoRoT and Kepler data on main-sequence stars and red...”
Published 2015-01-01
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6by Feast Michael W.“... stars, particularly asymptotic giant branch variables and R Coronae Borealis stars, is stressed...”
Published 2017-01-01
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7“... is verified for the most populated areas of the Hertzsprung-Russell diagram: main-sequence stars and red...”
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8by Claus Leitherer“... present a case study of the extraordinary star cluster and giant H II region in the blue compact galaxy II...”
Published 2020-02-01
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9“..., “The stars and a giant who chases after stars”, talks about story of a runner chasing the meteor. The main...”
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10by Goulet, Thomas“...) main sequence B stars, 4) B stars of luminosity class ranging from I to IV, 5) main sequence A stars, 6...”
Published 2010
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11by Hughes, Evan Eugene“...) 35 percent of the stars are generally giant stars of type MO or earlier and are not luminous enough...”
Published 1969
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12by Taylor S.F.“...] suggested the Kepler field may include an older population of stars. The tidal dissipation strength in stars...”
Published 2013-04-01
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13by I. A. Usenko, A. Yu. Kniazev, V. V. Kovtyukh, T. V. Mishenina, A. S. Miroshnichenko, D. G. Turner, Yu. I. Protsyuk“...] = −0.1±0.04 dex. The main sequence stars and B-giants have abundances of C, N, and Na close to the solar...”
Published 2018-10-01
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14by Nuñez, P. D., Scott, N. J., Mennesson, B., Absil, O., Augereau, J.-C., Bryden, G., ten Brummelaar, T., Ertel, S., Coudé du Foresto, V., Ridgway, S. T., Sturmann, J., Sturmann, L., Turner, N. J., Turner, N. H.“... in a sample of main sequence stars and sub-giants. Using the "jouvence" of the fiber linked unit...”
Published 2017
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15by Bennett, Michael Edward“... in stellar models. The s-process, which is a slow neutron-capture process that can occur in massive stars...”
Published 2011
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16by Ngo, Henry Hoang Khoi“... and the giant planet.</p> <p>In the third study, we search for stellar companions around stars that host...”
Published 2017
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19by Weistrop, Donna Etta“... to the method used. Having estimated the contributions to the star counts due to Population II stars and disk...”
Published 1971
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20by Murdoch, Kaylene A.“... solar-type stars and 10 giant International Astronomical Union radial-velocity standard stars...”
Published 2013
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