Zobrazeno 1 - 10
of 15
pro vyhledávání: '"V. F. Shvartsman"'
Autor:
M. Yu. Popova, A. V. Zhuravkov, V. F. Shvartsman, Gregory Beskin, I. N. Bernstein, V. N. Komarova, V. L. Plokhotnichenko, S. I. Neizvestny
Publikováno v:
Astronomical & Astrophysical Transactions. 13:13-17
We describe the hard/software MANIA complex for carrying out superfast photometry. A new type of time-code converter Quantochron allows us to measure arrival times of photons registered by a photodetector with time resolution up to 20 ns in 216 chann
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d389ea951e515a2b0d8e97bf3676500a
https://doi.org/10.1080/10556799708208109
https://doi.org/10.1080/10556799708208109
Publikováno v:
Astrophysics. 31:685-690
8. B. E. Markaryan, V. A. Lipovetskii, and Dzh. A. Stepanyan, Astrofizika, 15, 363 (1979). 9. B. E. Markaryan, V. A. Lipovetskii, and Dzh. A. Stepanyan, Astrofizika, 17, 619 (1981). i0. B. E. Markaryan, V. A. Lipovetskii, and Dzh. A. Stepanyan, Astro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ba2ba6c64f845d3c39aad881641d3f80
https://doi.org/10.1007/bf01012725
https://doi.org/10.1007/bf01012725
Publikováno v:
Symposium - International Astronomical Union. 130:129-137
In 1986 the programme “The Northern Cone of Metagalaxy” has been finished with the 6-meter Telescope. In the course of the programme redshifts of all very rich compact clusters of galaxies inside the cone with galactic latitude and indirect estim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b58435592c5469c64dc6f3119404bb3b
https://doi.org/10.1017/s0074180900135934
https://doi.org/10.1017/s0074180900135934
Autor:
V. N. Mansurov, L. A. Pustil'Nik, V. F. Shvartsman, V. S. Pavlova, A. K. Yakushev, G. S. Tsarevsky, O. A. Evseyev
Publikováno v:
Symposium - International Astronomical Union. 67:477-480
At the Special Astrophysical Observatory of the U.S.S.R., an experiment to detect super-rapid variability of brightness and polarization in a number of peculiar objects is being carried out. This includes the optical stars identified with X-ray sourc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8bf36f403e9cf927c349a17a0ed9f57c
https://doi.org/10.1017/s0074180900010640
https://doi.org/10.1017/s0074180900010640
Autor:
V. F. Shvartsman
Publikováno v:
Radiophysics and Quantum Electronics. 13:1428-1440
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9071732d1c5e7dcf37dc7b2e22cae9f2
https://doi.org/10.1007/bf01032996
https://doi.org/10.1007/bf01032996
Autor:
V. F. Shvartsman
Publikováno v:
Astrophysics. 6:159-163
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::35b4d9d11e99e5fab4272aa363971784
https://doi.org/10.1007/bf01007262
https://doi.org/10.1007/bf01007262
Autor:
V. F. Shvartsman
Publikováno v:
Astrophysics. 6:56-62
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2d6c33d8b5781e98a6170e37956b0db7
https://doi.org/10.1007/bf01002575
https://doi.org/10.1007/bf01002575
Autor:
V. L. Plakhotnichenko, S. I. Neizvestnyj, V. F. Shvartsman, L. A. Pustil'Nik, R. E. Gershberg, G. M. Beskin
Publikováno v:
International Astronomical Union Colloquium. 104:103-105
High time resolution monitoring of the UV Cet type flare stars has enabled as to detect flares with total duration of a few seconds and with energy output comparable to solar subflares. We find that the time scales of decay for such flares correspond
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::28e570d3d68fad5e7040944585741a08
https://doi.org/10.1017/s0252921100153916
https://doi.org/10.1017/s0252921100153916
Autor:
G. M. Beskin, V. L. Plakhotnichenko, R. E. Gershberg, L. A. Pustil'Nik, V. F. Shvartsman, S. N. Mitronova, S. I. Neizvestnyj
Publikováno v:
International Astronomical Union Colloquium. 104:95-97
A detailed analysis of 73 flares on UV Cet type stars observed at the 6 m telescope of the Special Astrophysical Observatory with 3x10–7 s time resolution shows no fine structures on flare light curves with time scales from 10–6 to 10–1 s.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9c8fa247f55355c095b64d4ae460e5ed
https://doi.org/10.1017/s0252921100153898
https://doi.org/10.1017/s0252921100153898
Publikováno v:
International Astronomical Union Colloquium. 104:99-101
We have studied the initial phases of 65 optical flares on UV Cet type stars with a time resolution of 3x10–7 s. Ninety per cent of these flares have rapid brightenings shorter than 10 s and several are shorter than 1 s. We detected on UV Cet the s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::70e65a623813b86cfeb263f7e03d6191
https://doi.org/10.1017/s0252921100153904
https://doi.org/10.1017/s0252921100153904