Spectroscopic and photometric studies of four W UMa-type eclipsing binaries
L Long, LY Zhang, XL Han, HP Lu… - Monthly Notices of the …, 2019 - academic.oup.com
We performed new photometric and spectroscopic studies on four W UMa-type eclipsing
binaries (V400 Lyr, V574 Lyr, V1033 Her and V1062 Her). The main aims were to determine …
binaries (V400 Lyr, V574 Lyr, V1033 Her and V1062 Her). The main aims were to determine …
Photometric study and absolute parameters of the short-period eclipsing binary HH Bootis
B Gürol, DH Bradstreet, Y Demircan, SH Gürsoytrak - New Astronomy, 2015 - Elsevier
We present the results of our investigation on the geometrical and physical parameters of
the W UMa type binary system HH Bootis from new CCD (BVRI) light curves and published …
the W UMa type binary system HH Bootis from new CCD (BVRI) light curves and published …
Photometry, period variations and light curve analysis of eclipsing binary V1191 Cyg
S Ostadnezhad, M Delband, A Hasanzadeh - New Astronomy, 2014 - Elsevier
New observations of the eclipsing binary system V1191 Cyg were carried out by using CCD
in BVR filters and new times of light minimum and new ephemeris were obtained. For the …
in BVR filters and new times of light minimum and new ephemeris were obtained. For the …
The first photometric investigation of the neglected short period binary DY CVn
Q ZhiNing, J LinQiao, L Jie, H YanFei, Y YuQuan - New Astronomy, 2017 - Elsevier
We present new photometric observations of the short period binary DY CVn. By using the
Wilson-Devinney code of 2013 version, we found that DY CVn is a shallow contact binary (f …
Wilson-Devinney code of 2013 version, we found that DY CVn is a shallow contact binary (f …
New Photometric Investigation of the Solar‐Type Shallow‐Contact Binary HH Bootis
J He, J Wang - Advances in Astronomy, 2019 - Wiley Online Library
The short‐period solar‐type contact binary HH Boo was monitored photometrically for about
8 years. It is found that the CCD light curves in the B, V, R, and I bands obtained in 2010 are …
8 years. It is found that the CCD light curves in the B, V, R, and I bands obtained in 2010 are …
[PDF][PDF] First Precision Photometric Observations and Analyses of the Totally Eclipsing, Solar Type Binary V573 Pegasi
RG Samec, DB Caton, DR Faulkner - Journal of the American …, 2018 - app.aavso.org
CCD VRcIc light curves of V573 Peg were taken 26 and 27 September and 2, 4, and 6
October, 2017, at the Dark Sky Observatory in North Carolina with the 0.81-m reflector of …
October, 2017, at the Dark Sky Observatory in North Carolina with the 0.81-m reflector of …