activity
20142024
most citedSpectroscopic Searches for Evolutionary Orbital Period Changes in WR+OB Binaries: The case of CQ Cep and CX Cep

9 citations · 34 across the 16 of their papers we have counts for

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astro-ph.SR2024

Radial velocities of narrow emission line components in the spectra of T Tauri stars

V. A. Kiryukhina, A. V. Dodin

We studied rotational modulation of the radial velocities of narrow emission lines in four classical T Tauri stars. We found that the previously declared shift of the mean velocity…

astro-ph.SR20241 cited

Discovery of a hot post-AGB star in Galactic globular cluster E3

R. Kumar, A. Moharana, S. Piridi +8

We report a new hot post-asymptotic giant branch (PAGB) star in the Galactic globular cluster (GC) E3, which is one of the first of the identified PAGB stars in a GC to show a bina…

astro-ph.SR20242 cited

The jet of BP Tau

A. V. Dodin, S. A. Potanin, M. A. Burlak +6

A strong global magnetic field of young low-mass stars and a high accretion rate are the necessary conditions for the formation of collimated outflows (jets) from these objects. Bu…

astro-ph.SR2024

Post-AGB candidate IRAS 02143+5852: Cepheid-like variability, three-layer circumstellar dust envelope and spectral features

N. P. Ikonnikova, M. A. Burlak, A. V. Dodin +8

We present the results of multicolour photometry, spectroscopic analysis and spectral energy distribution (SED) modelling for the post-AGB candidat…

astro-ph.SR2024

Spectroscopic Searches for Evolutionary Orbital Period Changes in WR+OB Binaries: the Case of WR 127 (Hen 3-1772)

I. A. Shaposhnikov, A. M. Cherepashchuk, A. V. Dodin +1

We aim at searching for secular evolution of the orbital period in the short-period binary system WR 127 (WN3b+O9.5V, ). We performed new low-resolution spectroscopic…

astro-ph.SR20241 cited

ZZ Tau IRS: a low mass UX Ori type star with strong wind

M. A. Burlak, A. V. Dodin, A. V. Zharova +7

The results of photometric, polarimetric and spectroscopic observations of the young star ZZ Tau IRS in the visible and near-infrared bands are presented. Against the continuum of…