GSC 01484-00665 , the SIMBAD biblio

2015AJ....149..146S - Astron. J., 149, 146 (2015/April-0)

First precision light curve analysis of the neglected extreme mass ratio solar-type binary HR Bootis.

SAMEC R.G., BENKENDORF B., DIGNAN J.B., ROBB R., KRING J. and FAULKNER D.R.

Abstract (from CDS):

HR Bootis is a neglected binary that is found to be a solar-type (G2V) extreme mass ratio binary (EMRB). It was discovered by Hanley & Shapley in 1940. Surprisingly, little has been published in the intervening years. In 1999 it was characterized by a 0.31587 day orbital period. Since that time it has been observed by various observers who have determined ∼20 timings of minimum light over the past ∼15,000 orbits. Our observations in 2012 represent the first precision curves in the BVRcIcJohnson-Cousins wavelength bands. The light curves have rather low amplitudes, averaging some 0.5 magnitudes, yet they exhibit total eclipses, which is typical of the rare group of solar-type EMRBs. An improved linear ephemeris was computed along with a quadratic ephemeris showing a decaying orbit, which indicates magnetic breaking may be occurring. The light curve solution reveals that HR Boo is a contact system with a somewhat low 21% Roche-lobe fill-out but a mass ratio of q = 4.09 (0.2444), which defines it as an EMRB. Two spots, both hot, were allowed to iterate to fit the light curve asymmetries. Their radii are 32° and 16°. Both are high-latitude polar spots indicative of strong magnetic activity. The shallow contact yet nearly equal component temperatures makes it an unusual addition to this group.

Abstract Copyright:

Journal keyword(s): binaries: close - binaries: eclipsing - stars: evolution - stars: individual: HR Boo

VizieR on-line data: <Available at CDS (J/AJ/149/146): table2.dat table3.dat table4.dat table5.dat table6.dat>

Simbad objects: 3

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2022.12.08-17:04:56

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