Results 241 to 250 of about 177,797 (288)
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Virtual Observatory for stellar astronomy
Astronomische Nachrichten, 2013AbstractThe principal idea of the Virtual Observatory is to achieve real transparency for astronomical data, similar to transparency for all the world's documents in the World Wide Web. In the Virtual Observatory, all the world's astronomical data is available from one's desktop.
Malkov, O., Zolotukhin, I.
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Astronomy Reports
We provide an analytic review of problems of the modern stellar astronomy. It mostly based on talks presented at the thirteenth annual conference on Modern Stellar Astronomy, held in Volgograd State University (Russia) in May 2023. The key topics for the review are Stars, Stellar Clusters and Associations, Interstellar Medium and Star Formation, Galaxy
O. Yu. Malkov +2 more
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We provide an analytic review of problems of the modern stellar astronomy. It mostly based on talks presented at the thirteenth annual conference on Modern Stellar Astronomy, held in Volgograd State University (Russia) in May 2023. The key topics for the review are Stars, Stellar Clusters and Associations, Interstellar Medium and Star Formation, Galaxy
O. Yu. Malkov +2 more
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Advances in Space Research, 1990
Abstract The properties of the X-ray emission from normal stars, i.e., single stars located on the main-sequence or giant branch, are reviewed. Theoretical attempts to explain the observed X-ray emission both from early as well as late type stars are presented and, in particular, coronal length scale determination from spatially unresolved data is ...
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Abstract The properties of the X-ray emission from normal stars, i.e., single stars located on the main-sequence or giant branch, are reviewed. Theoretical attempts to explain the observed X-ray emission both from early as well as late type stars are presented and, in particular, coronal length scale determination from spatially unresolved data is ...
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Far-infrared stellar astronomy
Symposium - International Astronomical Union, 1966The photometer with which I am presently observing stellar radiation responds in the wavelength band extending from 8 to 14 microns. I believe common usage places the boundary between the intermediate and far infrared at 10 microns. From the title of this paper one may therefore infer that what I say today is at least one-third wrong from the start.
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Solar-stellar astronomy working group summary
AIP Conference Proceedings, 1990The South Pole and other Antarctic stations offer unique possibilities for observations of the sun, stars and planets. Past, current and future use and options for such observations are considered. There is a clear need for more detailed information about observing conditions at the South Pole.
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Stellar Astronomy in the Warm Spitzer Era
AIP Conference Proceedings, 2007We consider the impact on the study of normal stars of large‐scale pointed and mapping observations at 3.6 μm and 4.5 μm with the Spitzer IRAC imager. Deep observations at these wave‐lengths are particularly sensitive to very cool stellar and substellar objects, both as companions to other stars and in the field.
Gillian R. Knapp +7 more
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Astronomy is stellar field for younger women
Physics World, 2003Photographs of theoretical physicists are usually few and far between in Britain's tabloid newspapers, but that was not the case last month when Stephen Hawking was pictured enjoying the company of lapdancers at Stringfellows night club in london. Hawking was on a night out with his assistant Mark and two nurses, and delighted Peter Stringfellow when ...
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Astrophysics and Stellar Astronomy
American Journal of Physics, 1971Thomas L. Swihart, Peter D. Noerdlinger
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Astrophysics and Stellar Astronomy
American Journal of Physics, 1970Thomas L. Swthart, F. R. Zabriskie
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