Serbian Astronomical Journal (Jan 2024)

Luminosity class of the symbiotic stars 4U1954+319 and ZZ CMi

  • Zamanov R.,
  • Stoyanov K.A.,
  • Latev G.,
  • Marti J.,
  • Takey A.,
  • Elhosseiny E.G.,
  • Christova M.D.,
  • Minev M.,
  • Vujčić V.,
  • Moyseev M.,
  • Marchev V.

DOI
https://doi.org/10.2298/SAJ240206002Z
Journal volume & issue
Vol. 2024, no. 208
pp. 41 – 46

Abstract

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We performed optical photometry and spectral observations of the symbiotic stars 4U1954+319 and ZZ CMi. For 4U1954+319, using high-resolution spectra, we, measure the equivalent widths of diffuse interstellar bands (DIBs) and estimate the interstellar reddening E(B-V ) = 0:83±0:09. Using the GAIA distances and our photometry, we find: (1) the absolute V -band magnitude MV =-5:23 ± 0:08 of 4U1954+319 and that the mass donor is a supergiant of luminosity class Ib, and (2) MV = -0:27±0:2 for ZZ CMi and that the mass donor is a giant of luminosity class III.

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