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Photopolarimetric activity of the Ae Herbig star SV Cep. / Rostopchina, A. N.; Grinin, V. P.; Shakhovskoǐ, D. N.; Thé, P. S.; Minikulov, N. Kh.

в: Astronomy Reports, Том 44, № 6, 01.01.2000, стр. 365-375.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Rostopchina, AN, Grinin, VP, Shakhovskoǐ, DN, Thé, PS & Minikulov, NK 2000, 'Photopolarimetric activity of the Ae Herbig star SV Cep', Astronomy Reports, Том. 44, № 6, стр. 365-375. https://doi.org/10.1134/1.163860

APA

Rostopchina, A. N., Grinin, V. P., Shakhovskoǐ, D. N., Thé, P. S., & Minikulov, N. K. (2000). Photopolarimetric activity of the Ae Herbig star SV Cep. Astronomy Reports, 44(6), 365-375. https://doi.org/10.1134/1.163860

Vancouver

Rostopchina AN, Grinin VP, Shakhovskoǐ DN, Thé PS, Minikulov NK. Photopolarimetric activity of the Ae Herbig star SV Cep. Astronomy Reports. 2000 Янв. 1;44(6):365-375. https://doi.org/10.1134/1.163860

Author

Rostopchina, A. N. ; Grinin, V. P. ; Shakhovskoǐ, D. N. ; Thé, P. S. ; Minikulov, N. Kh. / Photopolarimetric activity of the Ae Herbig star SV Cep. в: Astronomy Reports. 2000 ; Том 44, № 6. стр. 365-375.

BibTeX

@article{81c86eb9718745f8924e68d14499933e,
title = "Photopolarimetric activity of the Ae Herbig star SV Cep",
abstract = "We present the results of simultaneous UBVRI photometric and polarimetric observations of the Ae Herbig star SV Cep made in 1987-1998. Over these 11 years, only a single deep (ΔV > 1m) brightness minimum was observed. Near this minimum, the brightness decrease was accompanied by an increase of the linear polarization, as is typical of young UX Ori stars. The photometric observations of SV Cep indicate reversals of the color tracks in brightness minima, as is common for stars of this type, as well as variations of the slopes of the color tracks during and after minima. This provides evidence that the circumstellar dust clouds screening the star differ in their sizes and masses, and also in the optical properties of their dust particles. A Fourier analysis of the brightness variations of SV Cep (including data from the literature) confirms the presence of previously suspected activity cycles with periods P1 = 4000d and P2 = 670d. The polarimetric observations indicate that, along with the inverse correlation between the degree of linear polarization and brightness, the polarization parameters vary on characteristic time scales of 4000 and 1000 days. This suggests the existence of large-scale inhomogeneities in the circumstellar dust disk rotating about the star. {\textcopyright} 2000 MAIK {"}Nauka/Interperiodica{"}.",
author = "Rostopchina, {A. N.} and Grinin, {V. P.} and Shakhovskoǐ, {D. N.} and Th{\'e}, {P. S.} and Minikulov, {N. Kh}",
year = "2000",
month = jan,
day = "1",
doi = "10.1134/1.163860",
language = "English",
volume = "44",
pages = "365--375",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "6",

}

RIS

TY - JOUR

T1 - Photopolarimetric activity of the Ae Herbig star SV Cep

AU - Rostopchina, A. N.

AU - Grinin, V. P.

AU - Shakhovskoǐ, D. N.

AU - Thé, P. S.

AU - Minikulov, N. Kh

PY - 2000/1/1

Y1 - 2000/1/1

N2 - We present the results of simultaneous UBVRI photometric and polarimetric observations of the Ae Herbig star SV Cep made in 1987-1998. Over these 11 years, only a single deep (ΔV > 1m) brightness minimum was observed. Near this minimum, the brightness decrease was accompanied by an increase of the linear polarization, as is typical of young UX Ori stars. The photometric observations of SV Cep indicate reversals of the color tracks in brightness minima, as is common for stars of this type, as well as variations of the slopes of the color tracks during and after minima. This provides evidence that the circumstellar dust clouds screening the star differ in their sizes and masses, and also in the optical properties of their dust particles. A Fourier analysis of the brightness variations of SV Cep (including data from the literature) confirms the presence of previously suspected activity cycles with periods P1 = 4000d and P2 = 670d. The polarimetric observations indicate that, along with the inverse correlation between the degree of linear polarization and brightness, the polarization parameters vary on characteristic time scales of 4000 and 1000 days. This suggests the existence of large-scale inhomogeneities in the circumstellar dust disk rotating about the star. © 2000 MAIK "Nauka/Interperiodica".

AB - We present the results of simultaneous UBVRI photometric and polarimetric observations of the Ae Herbig star SV Cep made in 1987-1998. Over these 11 years, only a single deep (ΔV > 1m) brightness minimum was observed. Near this minimum, the brightness decrease was accompanied by an increase of the linear polarization, as is typical of young UX Ori stars. The photometric observations of SV Cep indicate reversals of the color tracks in brightness minima, as is common for stars of this type, as well as variations of the slopes of the color tracks during and after minima. This provides evidence that the circumstellar dust clouds screening the star differ in their sizes and masses, and also in the optical properties of their dust particles. A Fourier analysis of the brightness variations of SV Cep (including data from the literature) confirms the presence of previously suspected activity cycles with periods P1 = 4000d and P2 = 670d. The polarimetric observations indicate that, along with the inverse correlation between the degree of linear polarization and brightness, the polarization parameters vary on characteristic time scales of 4000 and 1000 days. This suggests the existence of large-scale inhomogeneities in the circumstellar dust disk rotating about the star. © 2000 MAIK "Nauka/Interperiodica".

UR - http://www.scopus.com/inward/record.url?scp=0034343465&partnerID=8YFLogxK

U2 - 10.1134/1.163860

DO - 10.1134/1.163860

M3 - Article

AN - SCOPUS:0034343465

VL - 44

SP - 365

EP - 375

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 6

ER -

ID: 126127483