Standard

Mechanism for cyclical activity of the Herbig Ae star BF Ori. / Grinin, V. P.; Rostopchina, A. N.; Barsunova, O. Yu.; Demidova, T. V.

In: Astrophysics, Vol. 53, No. 3, 2010, p. 367-372.

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

Harvard

Grinin, VP, Rostopchina, AN, Barsunova, OY & Demidova, TV 2010, 'Mechanism for cyclical activity of the Herbig Ae star BF Ori', Astrophysics, vol. 53, no. 3, pp. 367-372. https://doi.org/10.1007/s10511-010-9128-7

APA

Grinin, V. P., Rostopchina, A. N., Barsunova, O. Y., & Demidova, T. V. (2010). Mechanism for cyclical activity of the Herbig Ae star BF Ori. Astrophysics, 53(3), 367-372. https://doi.org/10.1007/s10511-010-9128-7

Vancouver

Grinin VP, Rostopchina AN, Barsunova OY, Demidova TV. Mechanism for cyclical activity of the Herbig Ae star BF Ori. Astrophysics. 2010;53(3):367-372. https://doi.org/10.1007/s10511-010-9128-7

Author

Grinin, V. P. ; Rostopchina, A. N. ; Barsunova, O. Yu. ; Demidova, T. V. / Mechanism for cyclical activity of the Herbig Ae star BF Ori. In: Astrophysics. 2010 ; Vol. 53, No. 3. pp. 367-372.

BibTeX

@article{0aed0b1d14ea402fb57f0edfae5ae0ad,
title = "Mechanism for cyclical activity of the Herbig Ae star BF Ori",
abstract = "The photometric activity of the star BF Ori, which belongs to the family of UX Ori-type stars, is studied. New data obtained with the ASAS robotic telescope confirm the existence of a cyclical component in the light curve for this star with a duration of roughly 11-12 years. The form of the photometric cycle resembles the theoretical light curves for a young binary system with a low-mass secondary component, and which is accreting matter from a surrounding common disk. Alternative mechanisms for the cyclical variability of UX Ori stars are also discussed.",
keywords = "stars, variable- individual, BF Ori",
author = "Grinin, {V. P.} and Rostopchina, {A. N.} and Barsunova, {O. Yu.} and Demidova, {T. V.}",
year = "2010",
doi = "10.1007/s10511-010-9128-7",
language = "English",
volume = "53",
pages = "367--372",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "3",

}

RIS

TY - JOUR

T1 - Mechanism for cyclical activity of the Herbig Ae star BF Ori

AU - Grinin, V. P.

AU - Rostopchina, A. N.

AU - Barsunova, O. Yu.

AU - Demidova, T. V.

PY - 2010

Y1 - 2010

N2 - The photometric activity of the star BF Ori, which belongs to the family of UX Ori-type stars, is studied. New data obtained with the ASAS robotic telescope confirm the existence of a cyclical component in the light curve for this star with a duration of roughly 11-12 years. The form of the photometric cycle resembles the theoretical light curves for a young binary system with a low-mass secondary component, and which is accreting matter from a surrounding common disk. Alternative mechanisms for the cyclical variability of UX Ori stars are also discussed.

AB - The photometric activity of the star BF Ori, which belongs to the family of UX Ori-type stars, is studied. New data obtained with the ASAS robotic telescope confirm the existence of a cyclical component in the light curve for this star with a duration of roughly 11-12 years. The form of the photometric cycle resembles the theoretical light curves for a young binary system with a low-mass secondary component, and which is accreting matter from a surrounding common disk. Alternative mechanisms for the cyclical variability of UX Ori stars are also discussed.

KW - stars

KW - variable- individual

KW - BF Ori

U2 - 10.1007/s10511-010-9128-7

DO - 10.1007/s10511-010-9128-7

M3 - Article

VL - 53

SP - 367

EP - 372

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 3

ER -

ID: 5179148