skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: TIME-SERIES SPECTROSCOPY OF THE ECLIPSING BINARY Y CAM WITH A PULSATING COMPONENT

Journal Article · · Astronomical Journal (Online)
; ; ; ;  [1]; ;  [2]
  1. Korea Astronomy and Space Science Institute, Daejeon 305-348 (Korea, Republic of)
  2. Department of Astronomy and Space Science, Sejong University, Seoul, 143-747 (Korea, Republic of)

We present the physical properties of the semi-detached Algol-type eclipsing binary Y Cam based on high resolution spectra obtained using the Bohyunsan Optical Echelle Spectrograph. This is the first spectroscopic monitoring data obtained for this interesting binary system, which has a δ Sct-type pulsating component. We obtained a total of 59 spectra over 14 nights from 2009 December to 2011 March. Double-lined spectral features from the hot primary and cool secondary components were well identified. We determined the effective temperatures of the two stars to be T{sub eff,1} = 8000 ± 250 K and T{sub eff,2} = 4629 ± 150 K. The projected rotational velocities are v{sub 1}sin i{sub 1} = 51 ± 4 km s{sup −1} and v{sub 2}sin i{sub 2} = 50 ± 10 km s{sup −1}, which are very similar to a synchronous rotation with the orbital motion. Physical parameters of each component were derived by analyzing our radial velocity data together with previous photometric light curves from the literature. The masses and radii are M{sub 1} = 2.08 ± 0.09 M{sub ⊙}, M{sub 2} = 0.48 ± 0.03 M{sub ⊙}, R{sub 1} = 3.14 ± 0.05 R{sub ⊙}, and R{sub 2} = 3.33 ± 0.05 R{sub ⊙}, respectively. A comparison of these parameters with the theoretical evolution tracks showed that the primary component is located between the zero-age main sequence and the terminal-age main sequence, while the low-mass secondary is noticeably evolved. This indicates that the two components have experienced mass exchange with each other and the primary has undergone an evolution process different from that of single δ Sct-type pulsators.

OSTI ID:
22520119
Journal Information:
Astronomical Journal (Online), Vol. 150, Issue 4; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1538-3881
Country of Publication:
United States
Language:
English

Similar Records

Time-series Spectroscopy of the Oscillating Eclipsing Algol System V392 Orionis
Journal Article · Tue Jan 01 00:00:00 EST 2019 · The Astronomical Journal (Online) · OSTI ID:22520119

Time-series Spectroscopy of the Oscillating Algol-type Binary AB Cas
Journal Article · Thu Jun 01 00:00:00 EDT 2017 · The Astronomical Journal (Online) · OSTI ID:22520119

Time-series spectroscopy of the pulsating eclipsing binary XX Cephei
Journal Article · Tue Mar 01 00:00:00 EST 2016 · The Astronomical Journal (Online) · OSTI ID:22520119