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

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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.

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Notes

  1. https://wise2.ipac.caltech.edu/docs/release/allsky/e.psup/sec4_ 4h.html#WISEZMA.

  2. https://irsa.ipac.caltech.edu/IRASdocs/iras.html.

  3. https://lambda.gsfc.nasa.gov/product/cobe/about_dirbe.cfm.

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ACKNOWLEDGMENTS

The authors express their gratitude to the referee for the careful reading of the manuscript and and the comments made that contribute to the improvement of the manuscript text.

Funding

N.I. is grateful for the support of the Foundation for the Development of Science under the President of the Republic of Azerbaijan (grant no. EIF-BGM-4-RFTF-1/2017-21/07/1). A.Kh. is grateful for the support of the RFBR grant 19-02-00311 a. I.I.R. and A.V.M. thank the Russian Science Foundation for partial financial support of work in terms of measurements of magnetic fields of stars (RSF grant 21-12-00147). A.V.M. is thankful for financial support of a grant from the President of the Russian Federation for young scientists—candidates of sciences no. 05-682.2021.6. Observations with telescopes of the SAO RAS are carried out with the support of the Ministry of Science and Higher Education of the Russian Federation (including agreement no. 05.619.21.0016, unique project identifier RFMEFI61919X0016).

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Authors and Affiliations

  1. Shamakhy Astrophysical Observatory named after Nasreddin Tusi, Azerbaijan National Academy of Sciences, AZ 5626, Shamakhy, Azerbaijan

    N. Z. Ismailov

  2. St. Petersburg University, 199034, St. Petersburg, Russia

    A. F. Kholtygin

  3. Special Astrophysical Observatory, Russian Academy of Sciences, 369167, Nizhnii Arkhyz, Russia

    I. I. Romanyuk & A. V. Moiseeva

  4. Central (Pulkovo) Astronomical Observatory, Russian Academy of Sciences, 196140, St. Petersburg, Russia

    M. A. Pogodin

Authors
  1. N. Z. Ismailov
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  2. A. F. Kholtygin
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  3. I. I. Romanyuk
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  4. M. A. Pogodin
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  5. A. V. Moiseeva
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Correspondence to N. Z. Ismailov or A. F. Kholtygin.

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Translated by T. Sokolova

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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

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  • DOI: https://doi.org/10.1134/S1990341321040064

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