Zobrazeno 1 - 10
of 30
pro vyhledávání: '"D. Yu. Tsvetkov"'
Autor:
D. Yu. Tsvetkov, V. P. Goranskij, E. A. Barsukova, A. F. Valeev, I. M. Volkov, N. N. Pavlyuk, S. Yu. Shugarov, N. I. Shatsky, O. V. Vozyakova, V. A. Echeistov
Publikováno v:
Astrophysical Bulletin. 77:407-414
Autor:
D. Yu. Tsvetkov, A. A. Belinsky, N. P. Ikonnikova, M. A. Burlak, I. M. Volkov, N. N. Pavlyuk, P. V. Baklanov, S. I. Blinnikov, M. G. Ushakova, V. A. Echeistov
Publikováno v:
Astronomy Letters. 48:209-221
Autor:
N. N. Pavlyuk, M. G. Ushakova, G. A. Borman, A. M. Tatarnikov, E. G. Larionova, D. Yu. Tsvetkov, A. A. Nikiforova, O. V. Vozyakova, N. I. Shatsky, S. I. Blinnikov, P. V. Baklanov
Publikováno v:
Astronomy Letters. 47:291-306
The results of UBVRIJHK photometry for the type II-P supernova SN 2018aoq in NGC 4151 obtained from April 4, 2018, to January 14, 2019, with several telescopes, including the 2.5-m telescope at the Caucasus Mountain Observatory of the Sternberg Astro
CCD BV RI photometry is presented for the type Ic-BL Supernovae 2016coi and 2018ebt. The shape of the light curves for both objects is typical for this class of SNe. A change of brightness decline rate at about 100 days after maximum light is observe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::25a7eaacb16766225a6bb61e2c22d64a
Autor:
Ivan S. Troitsky, N. N. Pavlyuk, O. V. Vozyakova, I. M. Volkov, D. Yu. Tsvetkov, P. V. Baklanov, A. A. Nikiforova, Yu. V. Troitskaya, S. Yu. Shugarov, N. I. Shatsky
Publikováno v:
Astronomy Letters. 44:315-323
We present the results of our UBVRI photometry for the type II-P supernova SN 2017eaw in NGC6946 obtained fromMay 14 to December 7, 2017, at several telescopes, including the 2.5-m telescope at the CaucasusHigh-Altitude Observatory of the SAIMSU. The
Autor:
M. Sh. Potashov, N.A. Huseynov, O. V. Khalilov, S. Yu. Shugarov, Vladimir Metlov, Kh. M. Mikailov, I. M. Volkov, V. L. Oknyansky, I. A. Alekberov, P. V. Baklanov, D. Yu. Tsvetkov, N. N. Pavlyuk
We present optical photometric observations of SN 2018aoq from 2 to 100 days after explosion, and 7 spectra at epochs from 11 to 71 days. The light curves and spectra are typical for SNe II-P. As previously reported, SN 2018aoq appears to be of inter
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3818e08baaa64dabab0c04d9d797b6f
http://arxiv.org/abs/1904.06586
http://arxiv.org/abs/1904.06586
Autor:
E. A. Barsukova, D. Yu. Tsvetkov, V. P. Goranskij, I. M. Volkov, A. F. Valeev, A. V. Zharova, Vladimir Metlov
Publikováno v:
Astrophysical Bulletin. 71:422-435
We present spectroscopy and multicolor photometry for the optical transient PSN J09093496+3307204 in the galaxy NGC2770, which has afterwards been transferred into the supernova phase and got the name SN2015bh. Medium-resolution spectral observations
Autor:
D. Yu. Tsvetkov, N. N. Pavlyuk
Publikováno v:
Astronomy Letters. 42:495-505
The distributions of supernovae of different types and subtypes along the radius and in z coordinate of galaxies have been studied. We show that among the type Ia supernovae (SNe Ia) in spiral galaxies, SNe Iax and Ia-norm have, respectively, the lar
Autor:
T. A. Lozinskaya, A. M. Tatarnikov, V. P. Arkhipova, A. V. Zharova, G. M. Rudnitskij, V. F. Esipov, N. P. Ikonnikova, Oleg V. Egorov, T. G. Sitnik, D. Yu. Tsvetkov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 432:2273-2283
The interstellar medium in the region of a family of cometary globules including the reflection nebula GM 2-39 has been analyzed basing on our observations with the slit spectrograph, the results of our previous observations with a Fabry-Perot interf
Autor:
E. Di Carlo, Nancy Elias-Rosa, Adriano Pietrinferni, Maria Teresa Botticella, Andrea Pastorello, D. L. Gorshanov, Stephen Smartt, Stefano Benetti, Valeri M. Larionov, A. A. Arkharov, Gabriella Raimondo, Kate Maguire, H. Navasardyan, Gaetano Valentini, M. Fiaschi, S. Spiro, Sergio Cristallo, D. Yu. Tsvetkov, G. Di Rico, Avet Harutyunyan, Stefano Valenti, Mauro Dolci, Enrico Cappellaro, Luca Zampieri, Giacomo Beccari
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 404:981-1004
We present new optical and near infrared (NIR) photometry and spectroscopy of the type IIP supernova, SN 2004et. In combination with already published data, this provides one of the most complete studies of optical and NIR data for any type IIP SN fr