onychomycosis
发表于 2025-3-21 16:39:47
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功多汁水
发表于 2025-3-21 22:02:37
Activity of Contact Binary Systems,nally called the “W UMa-type” systems. This limitation results mainly from a better knowledge of properties of cooler systems (i.e. with periods below about 0.5 – 0.6 days) but is also dictated by an expectation that only late-type stars can generate any magnetic activity.
perjury
发表于 2025-3-22 04:26:47
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Explosive
发表于 2025-3-22 07:55:12
Tidal Interactions of Close Binary Systems,mall orbital eccentricities (e.g. Young & Koniges 1977, Koch & Hrivnak 1981, Middelkoop & Zwaan 1982). There appears to be no such correlation for wide binary systems, which show a wide scatter of orbital eccentricities. This phenomenon is usually explained in terms of tidal interaction between the
expdient
发表于 2025-3-22 08:55:35
Wolf-Rayet Stars and Binarity,nformation on stellar masses, the motions and physics of interacting material streams connecting the stellar components and providing tests for binary stellar evolution models. The past decade has witnessed some significant changes to the picture of what constitutes a WR star and as to what role bin
PLIC
发表于 2025-3-22 13:41:19
Photometry of Active Algols, and most notably in U Cep have these disturbances been large enough to analyse quantitatively. From a study of the spectral distribution of light excesses and losses in U Cep, we derive properties of “equatorial bulges,” hot spot, and stream during periods of activity presumably associated with tra
Vulnerable
发表于 2025-3-22 17:32:20
From Algol to Beta Lyrae, be called .. β Lyrae is much more complicated, and some of the problems of revealing its structure are discussed. The best model available at the present considers β Lyrae as an Algol-type semi-detached system in a phase of fairly rapid mass transfer, i.e. younger than typical Algols. The most impo
DUCE
发表于 2025-3-23 01:08:27
Symbiotic Stars,uch models leads to the conclusion that symbiotic stars are likely to be main sequence or white dwarf stars accreting material from a red (super)giant primary. Recent observations of symbiotic stars confirm this notion, and three systems (CI Cyg — a red giant with an accreting main sequence star com
厨房里面
发表于 2025-3-23 05:03:12
Optical Characteristics of X-Ray Binaries,ew years and has now reached about 100 (Bradt & McClintock 1983), mainly as a result of refined X-ray positions obtained with the Ariel 5, SAS-3 and HEAO-1 satellites. In these sources there are good reasons to believe that the X-ray emission results from accretion onto a collapsed object, matter be
Fester
发表于 2025-3-23 09:29:13
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