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Photometric and Spectroscopic Study of Ten Low Mass Ratio Contact Binary Systems: Orbital Stability, O'Connell Effect and Infrared Calcium Line Filling

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Research in Astronomy and Astrophysics 2024年第8期24卷 214-224页

作者： Surjit S.Wadhwa Adam Popowicz Raúl Michel Petar Kosti? Oliver Vince Nick F.H.Tothill ain Y.de horta Miroslav D.Filipovi? School of Science Western Sydney University department of Electronics Electrical Engineering and MicroelectronicsSilesian University of Technology Instituto de Astronomía Astronomical Observatory

Low mass ratio contact binary systems are more likely to have unstable orbits and potentially *** addition,such systems exhibit characteristics such as starspots and high energy emissions (UV) suggestive of chromospheric and magnetic *** curve modeling of ten contact binary systems is *** were found to be of extreme low mass ratio ranging from 0.122 to 0.24 and three were found to be potentially unstable and possible merger *** of the infrared calcium absorption lines is a marker of increased chromospheric *** use the available Large Sky Area Multi-Object Fiber Spectroscopic Telescope spectra along with matched standard spectra (broadened for rotation) to measure the excess filling of the central core depression flux of the two main infrared calcium absorption linesλ8542 andλ*** find that all reported contact binaries have excess filling of the core flux in the infrared calcium *** of the systems reported were also observed by the Galaxy Evolution Explorer mission and we find that all three have features of excess ultraviolet emissions further adding evidence for increased chromospheric activity in low mass ratio contact *** of both orbital stability and absorption line filling is dependent on the determination of geometric and absolute parameters from light curve *** an insignificant number of contact binary light curves exhibit the O’Connell effect,usually attributed to *** discuss the inclusion of starspots in light curve solutions and how they influence the geometric and absolute parameters.

关键词： (stars:) binaries: eclipsing stars: chromospheres techniques: photometric

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Photometric Analysis of Three Potential Red Nova Progenitors

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Research in Astronomy and Astrophysics 2022年第10期22卷 103-110页

作者： Surjit S.Wadhwa ain de horta Miroslav D.Filipovic N.F.H.Tothill Bojan Arbutina Jelena Petrovic Gojko Djurasevic School of Science Western Sydney UniversityLocked Bag 1797PenrithNSW 2751Australia department of Astronomy Faculty of MathematicsUniversity of BelgradeStudentski trg 1611000 BelgradeSerbia Astronomical Observatory Volgina 711060 BelgradeSerbia

We present photometric analysis of three bright red nova progenitor contact binary systems:ASAS J082151-0612.6,TYC 7281-269-1 and TYC *** primary components in all three systems are solar-type low mass stars with radii somewhat larger than their zero age main sequence *** secondaries,as in most contact binary systems,have radii and luminosities well above their main sequence *** three have extremely low mass ratios ranging from 0.075 to 0.097 and two have high degrees of contact,in excess of 75%.All three have mass ratios and separations below the theoretical values for orbital *** activity,a hallmark of magnetic activity and magnetic braking,considered important in mediating angular momentum loss,is also *** three systems demonstrate the O’Connell effect,and all systems require the introduction of star spots for a better light curve *** addition,we show that ASAS J082151-0612.6 and TYC 7281-269-1 have a UV color excess in the range indicating high chromospheric *** measure of potential significant magnetic activity is X-ray luminosity;TYC 7275-1968-1 and probably also TYC 7281-269-1 have X-ray luminosity well above other contact binary *** conclude that it is likely that all three are unstable and hence are potential merger candidates.

关键词： (stars:)binaries eclipsing-techniques photometric-stars low-mass

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Photometric analysis of two extreme low mass ratio contact binary systems

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Research in Astronomy and Astrophysics 2021年第9期21卷 217-223页

作者： Surjit S.Wadhwa Nick F.H.Tothill ain Y.de horta Miroslav Filipovié School of Science Western Sydney UniversityLocked Bag 1797PenrithNSW 2751Australia

Multi-band photometry and light curve analysis for two newly recognized contact binary systems,TYC 6995-813-1 and NSVS 13602901,are *** were found to be of extreme low mass ratios 0.11 and 0.17,*** secondary components of both systems show evidence of considerable evolution with elevated densities as well as both luminosity and radii well above their main sequence *** in the absence of significant spot activity,at least one of the systems,TYC 6995-813-1,displays features of magnetic and chromospheric *** 6995-813-1 is also determined to be a potential merger candidate with its current separation near the theoretical instability separation.

关键词： stars:binaries:eclipsing stars:evolution stars:low-mass techniques:photometric

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Photometric and Spectroscopic Study of Two Low Mass Ratio Contact Binary Systems:CRTS J225828.7-121122 and CRTSJ030053.5+230139

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Research in Astronomy and Astrophysics 2023年第11期23卷 1-6页

作者： Surjit S.Wadhwa Jelena Petrović Nick F.H.Tothill ain Y.de horta Miroslav D.Filipović Gojko Djurašević School of Science Western Sydney UniversityLocked Bag 1797PenrithNSW 2751Australia Astronomical Observatory Volgina 711060 BelgradeSerbia

The study reports photometric and spectroscopic observations of two recently recognized contact binary *** systems show total eclipses and analysis of the light curves indicates both have very low mass ratios of less than *** derive absolute parameters from color and distance based calibrations and show that,although both have low mass ratios,they are likely to be in a stable orbit and unlikely to *** other respects,both systems have characteristics similar to other contact binaries with the secondary larger and brighter than their main sequence counterparts and we also find that the secondary is considerably denser than the primary in both systems.

关键词： (stars:)binaries:eclipsing stars:mass-loss techniques:photometric

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