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Large-scale photometric activity of UX Ori type stars. / Grinin, V. P.; Barsunova, O. Yu.; Shugarov, S. Yu.; Kroll, P.; Sergeev, S. G.

In: Astrophysics, Vol. 51, No. 1, 2008, p. 1-6.

Research output: Contribution to journal › Article › peer-review

Harvard

Grinin, VP, Barsunova, OY, Shugarov, SY, Kroll, P & Sergeev, SG 2008, 'Large-scale photometric activity of UX Ori type stars', Astrophysics, vol. 51, no. 1, pp. 1-6. https://doi.org/10.1007/s10511-008-0001-x

APA

Grinin, V. P., Barsunova, O. Y., Shugarov, S. Y., Kroll, P., & Sergeev, S. G. (2008). Large-scale photometric activity of UX Ori type stars. Astrophysics, 51(1), 1-6. https://doi.org/10.1007/s10511-008-0001-x

Vancouver

Grinin VP, Barsunova OY, Shugarov SY, Kroll P, Sergeev SG. Large-scale photometric activity of UX Ori type stars. Astrophysics. 2008;51(1):1-6. https://doi.org/10.1007/s10511-008-0001-x

Author

Grinin, V. P. ; Barsunova, O. Yu. ; Shugarov, S. Yu. ; Kroll, P. ; Sergeev, S. G. / Large-scale photometric activity of UX Ori type stars. In: Astrophysics. 2008 ; Vol. 51, No. 1. pp. 1-6.

BibTeX

@article{65451bd84fa34d36b8b83d8698c14361,
title = "Large-scale photometric activity of UX Ori type stars",
abstract = "Radical readjustments in the photometric activity of young stars owing to sudden changes in the circumstellar extinction are discussed using the light curves of two UX Ori type stars, CQ Tau and V1184 Tau, as examples. Changes of this sort can be caused by large deviations from axial symmetry in the distribution of circumstellar dust, as well as by large variations in the mass accretion rate in circumstellar disks. A large amount of dust may also appear in the vicinity of a young star owing to collisions of planetesimals.",
keywords = "stars, activity &mdash, individual, UX Ori type",
author = "Grinin, {V. P.} and Barsunova, {O. Yu.} and Shugarov, {S. Yu.} and P. Kroll and Sergeev, {S. G.}",
year = "2008",
doi = "10.1007/s10511-008-0001-x",
language = "English",
volume = "51",
pages = "1--6",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "1",

}

RIS

TY - JOUR

T1 - Large-scale photometric activity of UX Ori type stars

AU - Grinin, V. P.

AU - Barsunova, O. Yu.

AU - Shugarov, S. Yu.

AU - Kroll, P.

AU - Sergeev, S. G.

PY - 2008

Y1 - 2008

N2 - Radical readjustments in the photometric activity of young stars owing to sudden changes in the circumstellar extinction are discussed using the light curves of two UX Ori type stars, CQ Tau and V1184 Tau, as examples. Changes of this sort can be caused by large deviations from axial symmetry in the distribution of circumstellar dust, as well as by large variations in the mass accretion rate in circumstellar disks. A large amount of dust may also appear in the vicinity of a young star owing to collisions of planetesimals.

AB - Radical readjustments in the photometric activity of young stars owing to sudden changes in the circumstellar extinction are discussed using the light curves of two UX Ori type stars, CQ Tau and V1184 Tau, as examples. Changes of this sort can be caused by large deviations from axial symmetry in the distribution of circumstellar dust, as well as by large variations in the mass accretion rate in circumstellar disks. A large amount of dust may also appear in the vicinity of a young star owing to collisions of planetesimals.

KW - stars

KW - activity &mdash

KW - individual

KW - UX Ori type

U2 - 10.1007/s10511-008-0001-x

DO - 10.1007/s10511-008-0001-x

M3 - Article

VL - 51

SP - 1

EP - 6

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 1

ER -

ID: 5179237