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Spectral study of V565 Mon: probable FU Ori-like or chemically peculiar star
DOI: 10.1088/1674-4527/21/3/064
Bibcode: 2021RAA....21...64A
Andreasyan, Hasmik
We present a detailed spectroscopic study of pre-main sequence star V565 Mon, which is the illuminating star of the Parsamian 17 cometary nebula. Observations were performed with the 2.6 m telescope in Byurakan Astrophysical Observatory on 2018 February 15. Radial velocities and equivalent widths of the most prominent lines of V565 Mon are present…
2021
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Research in Astronomy and Astrophysics
AKARI
Gaia
3