Results 251 to 260 of about 2,962 (295)
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Far-infrared stellar astronomy

Symposium - International Astronomical Union, 1966
The 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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Modern Stellar Astronomy

Astronomy Reports, 2022
O. Yu. Malkov, E. V. Polyachenko
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Solar-stellar astronomy working group summary

AIP Conference Proceedings, 1990
The 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, 2007
We 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, 2003
Photographs 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, 1971
Thomas L. Swihart, Peter D. Noerdlinger
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Astrophysics and Stellar Astronomy

American Journal of Physics, 1970
Thomas L. Swthart, F. R. Zabriskie
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Stellar X-ray Astronomy with ROSAT

1988
We discuss the possibilities of stellar X-ray astronomy using the the next generation of X-ray telescopes onboard ROSAT. ROSAT will perform both an all sky survey at X-ray and XUV wavelengths exceeding the sensitivity of previous all sky surveys by orders of magnitude as well as pointed observations of specific targets.
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Gravitational-wave physics and astronomy in the 2020s and 2030s

Nature Reviews Physics, 2021
Matthew Bailes   +2 more
exaly  

Stellar Astronomy

Journal for the History of Astronomy, 1986
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