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20022025
most citedBlazar spectral variability as explained by a twisting inhomogeneous jet

199 citations · 1.8k across the 86 of their papers we have counts for

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astro-ph.SR2019★ 1 cited

Photometric and spectroscopic study of 5 pre-main sequence stars in the vicinity of NGC 7129

Evgeni H. Semkov, Sunay I. Ibryamov, Stoyanka P. Peneva

We present results from long-term optical photometric and spectroscopic observations of 5 pre-main sequence stars, located in the vicinity of the bight nebula NGC 7129. We obtained…

astro-ph.HE2019★ 30 cited

Investigating the multiwavelength behaviour of the flat spectrum radio quasar CTA 102 during 2013-2017

F. D'Ammando, C. M. Raiteri, M. Villata +94

We present a multiwavelength study of the flat-spectrum radio quasar CTA 102 during 2013-2017. We use radio-to-optical data obtained by the Whole Earth Blazar Telescope, 15 GHz dat…

astro-ph.SR2019

New four-color optical photometry of the young stars V521 Cyg and FHO 27

Sunay Ibryamov, Evgeni Semkov

Results from new BVRI photometric observations of the pre-MS stars V521 Cyg and FHO 27 collected during the period from February 2015 to July 2019 are presented. These stars are em…

astro-ph.SR2019★ 2 cited

Photometry of Symbiotic Stars - XIV

M. Sekeráš, A. Skopal, S. Shugarov +7

We present new multicolour UBVRcIc photometric observations of symbiotic stars, EG And, Z And, BF Cyg, CH Cyg, CI Cyg, V1016 Cyg, V1329 Cyg, AG Dra, RS Oph, AG Peg, AX Per, and the…

astro-ph.SR2019★ 8 cited

Diagnosing the Clumpy Protoplanetary Disk of the UXor Type Young Star GM Cephei

P. C. Huang, W. P. Chen, M. Mugrauer +29

UX Orionis stars (UXors) are Herbig Ae/Be or T Tauri stars exhibiting sporadic occultation of stellar light by circumstellar dust. GM\,Cephei is such a UXor in the young (~M…

astro-ph.HE2019★ 25 cited

Optical Variability of TeV Blazars on long time-scales

Haritma Gaur, Alok C. Gupta, R. Bachev +12

We present the results of photometric observations of three TeV blazars, 3C 66A, S5 0954+658 and BL Lacertae, during the period 2013--2017. Our extensive observations were performe…