Results 281 to 290 of about 547,732 (336)
Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run. [PDF]
Chaudhary SS+52 more
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Cosmic mysteries and the hydrogen 21-cm line: bridging the gap with lunar observations. [PDF]
Fialkov A, Gessey-Jones T, Dhandha J.
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Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky
Gilbert E+35 more
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Identification of a turnover in the initial mass function of a young stellar cluster down to 0.5 MJ
De Furio M+13 more
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Information seeking behaviour of astronomy/astrophysics scientists
ASLIB Proceedings, 2013Purpose – The purpose of this study is to examine different aspects of information seeking behaviour, and specifically the information seeking behaviour and information needs of Indian astronomy/astrophysics academics, including the relationship between ...
H. Sahu, Surya Nath Singh
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Astronomy and astrophysics with neutrinos
Physics Today, 2008Traversing cosmological distances without bending or energy loss, high-energy neutrinos are messengers from extreme astrophysical environments.
S. R. Klein, Francis Halzen
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Space Astronomy and Astrophysics
Physics Today, 1991Nearly everything we know about the cosmos comes from studying celestial electromagnetic radiation over roughly 16 decades of wavelength from radio to gamma ray. But most radiation is totally absorbed by our atmosphere—only radio and optical waves penetrate to Earth, and even these are subject to distortion or interference.
Claude R. Canizares, Blair D. Savage
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Astronomy and Astrophysics for the 1980s
Physics Today, 1982Astronomy is in a golden age. Discoveries since 1960 include quasars (1963), the cosmic microwave background radiation (1965), pulsars (1967), neutronstar binaries (1970), superluminal expansion of radio sources (1971), solar coronal holes (1973), evidence for gravitational radiation from a binary pulsar (1974), anomalous solar neutrino flux (1976), a ...
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Astronomy + Physics = Astrophysics [PDF]
In Chapter 1 we sought to give an introduction to classical astronomy with some historical remarks. In the same spirit we now turn to the astrophysical investigation of the Sun and stars. The latter we consider in the first place as individuals. Part III will deal with the internal constitution and evolution of stars and with stellar systems, galaxies,
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