Zobrazeno 1 - 4
of 4
pro vyhledávání: '"G. M. Rudnitski"'
Autor:
I. E. Val'tts, Willem A. Baan, A. V. Pogodin, O. S. Bayandina, Norbert Bartel, A. Z. Vorobyov, V. A. Molodtsov, G. M. Rudnitski, A. P. Lobanov, A. G. Rudnitski, David L. Jauncey, N. S. Kardashev, Hiroshi Imai, E. N. Filippova, Philip G. Edwards, Mikhail M. Lisakov, V. A. Soglasnov, Michael D. Johnson, A. V. Alakoz, V. E. Babyshkin, A. E. Shirshakov, José L. Gómez, Carl R. Gwinn, A. M. Sobolev, Tuomas Savolainen, P. A. Voitsik, G. Giovannini, B. S. Novikov, M. E. Churikova, M. V. Popov, Stan Kurtz, T. V. Smirnova, Kirill Sokolovsky, A. S. Andrianov, V. V. Khartov, M. I. Artyukhov, A. S. Privesenzev, V. I. Shishov, Yuri Y. Kovalev
Publikováno v:
SOLAR SYSTEM RESEARCH. 51(7):535-554
The RadioAstron ground-space interferometer provides the highest angular resolution achieved now in astronomy. The detection of interferometric fringes from quasars with this angular resolution on baselines of 100–200 thousand km suggests the brigh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8c2638c791fd979b7b46874e9ce13398
https://doi.org/10.1134/S0038094617070085
https://doi.org/10.1134/S0038094617070085
Autor:
G. M. Rudnitskij
Publikováno v:
Odessa Astronomical Publications, Vol 7, Iss 1, Pp 33-36 (2017)
Sources of molecular maser radio emission in envelopes of late-type variable stars (red giants and supergiants) are considered. Radio and optical data on asymmetry of mass loss process in red giants are briefly reviewed. Main attention is paid to mas
Externí odkaz:
https://doaj.org/article/f7d08441a78f4a329a6605d3f47daf55
Autor:
L. S. Kudashkina, G. M. Rudnitskij
Publikováno v:
Odessa Astronomical Publications, Vol 7, Iss 1, Pp 66-69 (2017)
The shapes of light curves of Mira-type variable stars is analyzed. It is shown that some features of the light curves may be explained by passage of shock waves in the stars' atmospheres. In particular, it is noted that "steps" of the ascending bran
Externí odkaz:
https://doaj.org/article/8ae0a855b2304649bf3ef74e9493097b
Autor:
G. M. Rudnitskij
Publikováno v:
Odessa Astronomical Publications, Vol 18, Iss 0, Pp 90-94 (2017)
The results of monitoring of a sample of late-type variable stars (Mira Ceti-type and semiregulars) are reported. Since 1980 a sample of 60 stars has been observed in the maser line of the H2O molecule at a wavelength of 1.35 cm. These observations a
Externí odkaz:
https://doaj.org/article/08c9e6c593274706b22011469a9995e0