27 citations · 54 across the 7 of their papers we have counts for
7 papers
Veiling of Photosphere Lines in the Spectra of UX ORI Stars at Deep Light Minima. I. The Star RR Tau
P. O. Dimitrieva, L. V. Tambovtseva, V. P. Grinin
The spectra of RR Tau star, which belongs to the family of young irregular variable UX Ori type stars, in its different brightness states have been studied using a comparative anal…
Clumpy accretion as a possible reason of prolonged eclipses of UX~Ori type stars
Vladimir Grinin, Tatiana Demidova
The paper proposes a model of deep and prolonged eclipses of young stars of the UX~Ori type. Some of these events continue for decades and existing models cannot explain them. Our…
UX Ori Stars Eclipses by Large-Scale Disc Perturbations
S. G. Shulman, V. P. Grinin
We simulate the polarized radiative transfer in vicinities of the UX Ori type stars during their minima. Our model of an eclipse by an extended disc perturbation generalizes the co…
SPH simulations of structures in protoplanetary disks
Tatiana Demidova, Vladimir Grinin
The hydrodynamic models of the protoplanetary disk, which perturbed by the embeded low-mass companion, were calculated by our modification of GADGET-2 code. The cases of circular a…
On the nature of the azimuthal asymmetry of protoplanetary disks observed pole-on. The case LkHa 101
Tatiana Demidova, Vladimir Grinin
The model of a protoplanetary disk of a star with a low-mass companion (), moving on a circular orbit, which slightly inclined to the disk plane ()…
Asymmetric Illumination of a Circumbinary Disk in the Presence of a Low-Mass Companion
T. Demidova, V. Grinin, N. Sotnikova
The model of an young star with a protoplanetary disk and a low-mass companion, which is moving on a circular orbit, inclined to the disk plane, is considered. The hydrodynamic mod…
An active asteroid belt causing the UX Ori phenomenon in RZ Psc
W. J. de Wit, V. P. Grinin, I. S. Potravnov +3
We report the discovery of mid-infrared excess emission in the young object RZ Psc. The excess constitutes ~8% of its Lbol, and is well fit by a single 500K black-body implying a d…