Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Nadjip, A."'
Autor:
Bizyaev, D., Tatarnikov, A. M., Shatsky, N. I., Nadjip, A. E., Burlak, M. A., Vozyakova, O. V.
We perform near-infrared photometry of a large sample of 49 superthin edge-on galaxies. These galaxies are selected based on optical photometry because of high radial-to-vertical scale ratio in their stellar disks. The Near Infrared (NIR) H and K obs
Externí odkaz:
http://arxiv.org/abs/2003.09842
Autor:
Dodin, A., Grankin, K., Lamzin, S., Nadjip, A., Safonov, B., Shakhovskoi, D., Shenavrin, V., Tatarnikov, A., Vozyakova, O.
Publikováno v:
MNRAS, Vol. 482, p. 5524 (2019)
Results of $UBVRIJHKLM$ photometry and $VRI$ polarimetry of a young star RW Aur A observed during unprecedented long and deep (up to $\Delta V \approx 5$ mag) dimming events in 2010-11 and 2014-18 are presented. The polarization degree $p$ of RW Aur
Externí odkaz:
http://arxiv.org/abs/1811.00449
Autor:
Nadjip, A. E., Tatarnikov, A. M., Toomey, D. W., Shatsky, N. I., Cherepashchuk, A. M., Lamzin, S. A., Belinski, A. A.
Publikováno v:
Astroph. Bull, 72, issue 3, p.349, 2017
ASTRONIRCAM is a cryogenic-cooled slit spectrograph for the spectral range 1-2.5 mkm installed at the Nasmyth focus of the 2.5-meter telescope of the Caucasian observatory of Sternberg Astronomical Institute of Lomonosov Moscow State University. The
Externí odkaz:
http://arxiv.org/abs/1706.08959
Autor:
S. A. Lamzin, A. M. Tatarnikov, D. W. Toomey, N. I. Shatsky, A. Belinski, A. M. Cherepashchuk, A. E. Nadjip
Publikováno v:
Astrophysical Bulletin. 72:349-362
ASTRONIRCAM is a cryogenic-cooled slit camera-spectrograph for the spectral range 1–2.5 μm installed at the Nasmyth focus of the 2.5-meter telescope of the Caucasian observatory of the Sternberg Astronomical Institute of Lomonosov Moscow State Uni
Autor:
S. A. Lamzin, V. I. Shenavrin, A. V. Dodin, A. M. Tatarnikov, K. N. Grankin, O. V. Vozyakova, A. E. Nadjip, D. N. Shakhovskoi, Boris Safonov
Results of $UBVRIJHKLM$ photometry and $VRI$ polarimetry of a young star RW Aur A observed during unprecedented long and deep (up to $\Delta V \approx 5$ mag) dimming events in 2010-11 and 2014-18 are presented. The polarization degree $p$ of RW Aur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d19dd54293dd346273180aadd578f4d
http://arxiv.org/abs/1811.00449
http://arxiv.org/abs/1811.00449
Akademický článek
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Autor:
Maslov, I., Nadjip, A.1, Taranova, O.1, Tatarnikov, A.1 andrey.tatarnikov@gmail.com, Shenavrin, V.1
Publikováno v:
Astrophysics. Sep2014, Vol. 57 Issue 3, p370-374. 5p.
Publikováno v:
Astrophysics. 57:370-374
Photometric data in the JHKLM near infrared bands obtained in 1999-2000 are presented for the long-period eclipsing system e Aur. The time of secondary eclipse (when the F21 supergiant eclipses a dust disk surrounding the more massive component of th
Autor:
Dodin, A, Grankin, K, Lamzin, S, Nadjip, A, Safonov, B, Shakhovskoi, D, Shenavrin, V, Tatarnikov, A, Vozyakova, O
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Feb2019, Vol. 482 Issue 4, p5524-5541, 18p
Autor:
S. V. Fomin, M. V. Kozin, G. M. Rudnitskij, E. E. Lekht, M. I. Pashchenko, A. E. Nadjip, V. F. Esipov
Publikováno v:
Symposium - International Astronomical Union. 191:201-206
Since 1994, observations of a sample of about 20 Mira Ceti-type and semiregular variables have been carried out in three spectral ranges: radio (H2O maser line λ = 1.35 cm), optical (spectroscopy and UBV photometry) and infrared (JHKLM photometry).