Zobrazeno 1 - 10
of 27
pro vyhledávání: '"D. N. Shakhovskoi"'
Autor:
N. V. Efimova, A. A. Arkharov, V. P. Grinin, A. N. Rostopchina-Shakhovskaya, D. N. Shakhovskoi, V. M. Larionov, S. A. Klimanov, D. L. Gorshanov
Publikováno v:
Astronomy Reports. 66:236-244
Autor:
V. I. Shenavrin, V. P. Grinin, D. N. Shakhovskoi, S. P. Belan, T. V. Demidova, A. N. Rostopchina-Shakhovskaya
Publikováno v:
Astronomy Reports. 61:38-46
The results of ~15 years of photometric observations of the UX Ori star SV Cep in the near-infrared (JHKL) are presented. They demonstrate the presence of a cyclic component with a period of ~7 years in the variations of the IR fluxes. This is clearl
Autor:
T. V. Demidova, V. P. Grinin, S. P. Belan, D. N. Shakhovskoi, A. N. Rostopchina-Shakhovskaya, V. I. Shenavrin
Publikováno v:
Astronomy Reports. 60:753-767
This paper continues a study of the photometric activity of UX Ori stars in the optical and near-infrared (JHKLM bands) initiated in 2000. For comparison, the list of program stars contains two Herbig Ae stars that are photometrically quiet in the op
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
Publikováno v:
Solar System Research. 47:185-188
Two-year BVRI polarimetric monitoring of the exoplanet system 51 Peg has been carried out, indicating that there is no orbital phase-dependent periodic variability in linear polarization with amplitudes greater than 0.04% in the R and I bands. The me
Publikováno v:
Astrophysics. 55:147-155
In a prolonged study (about 30 years) of the photometric activity of WW Vul we have discovered unusual eclipses in the light curve of this star. They last 2-3 years and repeat with a period of 13.9 years. One nontrivial feature of these eclipses is t
Publikováno v:
Astrophysics. 50:467-487
The results of the high-resolution long-term spectral monitoring of the Herbig Ae star HD 31648 in the regions of emission Hα line, Na I D resonance lines and OI 7774 lines are presented. We confirmed the conclusion, made in previous papers, that th
Publikováno v:
Astrophysics. 50:26-39
Results from simultaneous spectral and photometric monitoring of the Herbig Ae star CQ Tau in the neighborhood of the Hα and resonance sodium doublet Na I D lines are presented. It is shown that the inner structure of the accretion disk of CQ Tau is
Publikováno v:
Astronomy Reports. 51:55-66
Publikováno v:
Astrophysics. 49:151-163
Results of simultaneous spectral and photometric monitoring of the Ae Herbig star WW Vul in the neighborhoods of the Ha line and the sodium NaI D resonance doublet are reported. It is shown that the spectral variability of the star is caused mainly b