THE EMISSION-LINE DUSTY OBJECT IRAS 07080+0605, A LESS-EVOLVED EXAMPLE OF THE RED RECTANGLE

Автор(и)

  • S A. Khokhlov Physical-Technical Faculty, Al-Farabi Kazakh National University, Казахстан
  • A. S. Miroshnichenko Department of Physics and Astronomy, University of North Carolina at Greensboro, США
  • S. V, Zharikov Institute for Astronomy, Universidad Nacional Autónoma de M´ exico, Мексика
  • N. Manset Canada-France-Hawaii Corporation, США
  • O. V. Zakhozhay Main Astronomical Observatory, National Academy of Sciences of Ukraine, Україна
  • I. O. Bilinskyi Department of Astronomical Science, The Graduate University for Advanced Studies, Японія
  • K. N. Grankin Crimean Astrophysical Observatory, Україна
  • A. V. kusakin Fesenkov Astrophysical Institute, Казахстан
  • C. T. Omarov Fesenkov Astrophysical Institute, Казахстан
  • R. I, Kokumbaeva Fesenkov Astrophysical Institute, Казахстан
  • I. V. Reva Fesenkov Astrophysical Institute, Казахстан
  • D. Korcakova Astronomical Institute of Charles University, Чехія
  • I. A. Usenko Astronomical Observatory, Odessa National University, Mykolaiv Astronomical Observatory Research Institute, Україна
  • A. K. Kuratova Physical-Technical Faculty, Al-Farabi Kazakh National University, Казахстан

DOI:

https://doi.org/10.18524/1810-4215.2020.33.216403

Ключові слова:

Stars, emission-line, Be, evolution, circumstellar matter, binaries, general

Анотація

The all-sky survey conducted by
the InfraRed Astronomical Satellite (IRAS) in the
1980’s discovered many objects with infrared excesses
whose nature has not been explored until recently.
IRAS07080+0605 is one of those identified in the
visual spectral range with an early-type star, which
shows the B[e] phenomenon. The object is puzzling,
because it exhibits one of the strongest infrared
excesses associated with a star of one of the lowest
surface temperatures (∼8500 K) among objects with
the B[e] phenomenon, an apparent combination of
spectral features of dwarfs and supergiants, and
the absence of a surrounding optical nebula. Our
photometric and spectroscopic study shows that the
object’s properties are similar to those of the famous
Red Rectangle proto-planetary nebula. In this paper
we describe our findings and hypotheses about the
nature and evolutionary status of IRAS07080+0605

Посилання

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Опубліковано

2020-11-16

Номер

Том 33 (2020)

Розділ

Астроінформатика

Ліцензія

Авторське право (c) 2020 Odessa Astronomical Publications

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