ASAS J113031-0101.9 , the SIMBAD biblio

ASAS J113031-0101.9 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST18:13:20


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in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2007MNRAS.382..393R 55       D     X         2 9 68 The short-period end of the contact binary period distribution based on the All-Sky Automated Survey. RUCINSKI S.M.
2009IBVS.5886....1P 2         O           2 8 ASAS J071829-0336.7: short-period end for contact binaries redefined. PRIBULLA T., VANKO M. and HAMBALEK L.
2009BAVSR..58..258G         O           12 0 Aus den IBVS: 5870, 5871, 5872, 5873, 5874, 5875, 5877, 5878, 5880, 5882, 5884, 5886, 5887, 5888, 5889 und 5890. GRIMM W.
2011A&A...528A..90N viz 38           X         1 61 82 Short period eclipsing binary candidates identified using SuperWASP. NORTON A.J., PAYNE S.G., EVANS T., et al.
2011AJ....142..117S viz 15       D               1 30 13 UBVRcIc analysis of the recently discovered totally eclipsing extreme mass ratio binary V1853 Orionis, and a statistical look at 25 other extreme mass ratio solar-type contact binaries. SAMEC R.G., LABADORF C.M., HAWKINS N.C., et al.
2014ApJS..213....9D viz 16       D               1 46794 385 The Catalina surveys periodic variable star catalog. DRAKE A.J., GRAHAM M.J., DJORGOVSKI S.G., et al.
2015MNRAS.446..510K 56       D     X         2 55 18 Photometry and Hα studies of a low-mass-ratio overcontact binary ASAS J082243+1927.0. KANDULAPATI S., DEVARAPALLI S.P. and PASAGADA V.R.
2015AJ....150...69Y 175       D     X         5 48 69 Deep, low mass ratio overcontact binary systems. XIV. A statistical analysis of 46 sample binaries. YANG Y.-G. and QIAN S.-B.
2018AJ....156..241H viz 16       D               1 311114 199 A first catalog of variable stars measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS). HEINZE A.N., TONRY J.L., DENNEAU L., et al.
2018RAA....18..129K 16       D               1 46 13 NSVS 2569022: a peculiar binary among W UMa stars with extremely small mass ratios. KJURKCHIEVA D.P., POPOV V.A. and PETROV N.I.

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