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Relict Gas-and-Dust Disks Around AB Stars in the Orion Nebula. I. IR Excesses. / Ismailov, N. Z.; Kholtygin, A. F.; Romanyuk, I. I.; Pogodin, M. A.; Moiseeva, A. V.

в: Astrophysical Bulletin, Том 76, № 4, 10.2021, стр. 415-423.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Ismailov, NZ, Kholtygin, AF, Romanyuk, II, Pogodin, MA & Moiseeva, AV 2021, 'Relict Gas-and-Dust Disks Around AB Stars in the Orion Nebula. I. IR Excesses', Astrophysical Bulletin, Том. 76, № 4, стр. 415-423. https://doi.org/10.1134/S1990341321040064

APA

Ismailov, N. Z., Kholtygin, A. F., Romanyuk, I. I., Pogodin, M. A., & Moiseeva, A. V. (2021). Relict Gas-and-Dust Disks Around AB Stars in the Orion Nebula. I. IR Excesses. Astrophysical Bulletin, 76(4), 415-423. https://doi.org/10.1134/S1990341321040064

Vancouver

Ismailov NZ, Kholtygin AF, Romanyuk II, Pogodin MA, Moiseeva AV. Relict Gas-and-Dust Disks Around AB Stars in the Orion Nebula. I. IR Excesses. Astrophysical Bulletin. 2021 Окт.;76(4):415-423. https://doi.org/10.1134/S1990341321040064

Author

Ismailov, N. Z. ; Kholtygin, A. F. ; Romanyuk, I. I. ; Pogodin, M. A. ; Moiseeva, A. V. / Relict Gas-and-Dust Disks Around AB Stars in the Orion Nebula. I. IR Excesses. в: Astrophysical Bulletin. 2021 ; Том 76, № 4. стр. 415-423.

BibTeX

@article{499e2a1577334845b245b5aecf3af047,
title = "Relict Gas-and-Dust Disks Around AB Stars in the Orion Nebula. I. IR Excesses",
abstract = "Abstract: This paper is devoted to the study of gas-and-dust disks around young AB stars in the association Orion OB1. The observed spectral flux values of these stars in the wavelength range of 0.36–100 μm are determined. We used the results of multicolor photometric observations in the UBVRIJHK-bands, as well as data from the WISE and IRAS catalogs. It is shown that many program stars have radiation excesses in the far IR range. It is assumed that such an excess may be the result of the formation of a gas-dust disk around the program stars similar to those for Vega-type stars.",
keywords = "infrared: stars, stars: magnetic field, stars: pre-main sequence, stars: variables: T Tauri, Herbig Ae/Be",
author = "Ismailov, {N. Z.} and Kholtygin, {A. F.} and Romanyuk, {I. I.} and Pogodin, {M. A.} and Moiseeva, {A. V.}",
note = "Ismailov, N.Z., Kholtygin, A.F., Romanyuk, I.I. et al. Relict Gas-and-Dust Disks Around AB Stars in the Orion Nebula. I. IR Excesses. Astrophys. Bull. 76, 415–423 (2021). https://doi.org/10.1134/S1990341321040064",
year = "2021",
month = oct,
doi = "10.1134/S1990341321040064",
language = "English",
volume = "76",
pages = "415--423",
journal = "Astrophysical Bulletin",
issn = "1990-3413",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "4",

}

RIS

TY - JOUR

T1 - Relict Gas-and-Dust Disks Around AB Stars in the Orion Nebula. I. IR Excesses

AU - Ismailov, N. Z.

AU - Kholtygin, A. F.

AU - Romanyuk, I. I.

AU - Pogodin, M. A.

AU - Moiseeva, A. V.

N1 - Ismailov, N.Z., Kholtygin, A.F., Romanyuk, I.I. et al. Relict Gas-and-Dust Disks Around AB Stars in the Orion Nebula. I. IR Excesses. Astrophys. Bull. 76, 415–423 (2021). https://doi.org/10.1134/S1990341321040064

PY - 2021/10

Y1 - 2021/10

N2 - Abstract: This paper is devoted to the study of gas-and-dust disks around young AB stars in the association Orion OB1. The observed spectral flux values of these stars in the wavelength range of 0.36–100 μm are determined. We used the results of multicolor photometric observations in the UBVRIJHK-bands, as well as data from the WISE and IRAS catalogs. It is shown that many program stars have radiation excesses in the far IR range. It is assumed that such an excess may be the result of the formation of a gas-dust disk around the program stars similar to those for Vega-type stars.

AB - Abstract: This paper is devoted to the study of gas-and-dust disks around young AB stars in the association Orion OB1. The observed spectral flux values of these stars in the wavelength range of 0.36–100 μm are determined. We used the results of multicolor photometric observations in the UBVRIJHK-bands, as well as data from the WISE and IRAS catalogs. It is shown that many program stars have radiation excesses in the far IR range. It is assumed that such an excess may be the result of the formation of a gas-dust disk around the program stars similar to those for Vega-type stars.

KW - infrared: stars

KW - stars: magnetic field

KW - stars: pre-main sequence

KW - stars: variables: T Tauri, Herbig Ae/Be

UR - http://www.scopus.com/inward/record.url?scp=85122818096&partnerID=8YFLogxK

U2 - 10.1134/S1990341321040064

DO - 10.1134/S1990341321040064

M3 - Article

AN - SCOPUS:85122818096

VL - 76

SP - 415

EP - 423

JO - Astrophysical Bulletin

JF - Astrophysical Bulletin

SN - 1990-3413

IS - 4

ER -

ID: 95512674