partly supported by the research fund of the University of Shumen,Bulgaria。
This paper reports results from our long-term BV(RI)_(c) photometric CCD observations of eight pre-main sequence stars collected from 2008 June to 2022 October.These stars are located in the young open cluster Trumple...
partly supported by the National RI Roadmap Project(contracts D01-383/18.12.2020 and D01-176/29.07.2022)of the Ministry of Education and Science of the Republic of Bulgaria。
In this paper results from the optical photometric observations of the pre-main sequence star V1180 Cas are reported.The star is a young variable associated with the dark cloud Lynds 1340,located at a distance of 600 ...
The results of optical spectroscopic monitoring observations of a young binary system, Z CMa, are presented in this study. Z CMa consists of a Herbig Be star and an FU Orionis object, and it shows irregular light vari...
partly supported by the National Science Fund of the Ministry of Education and Science of Bulgaria under grant DN 18-10/2017;funds of the project RD-08-125/2021 of the University of Shumen。
Results from optical CCD photometric observations of 13 pre-main-sequence stars collected during the period from February 2007 to November 2020 are presented.These stars are located in the association Cepheus OB3,in t...
supported by the RA MES State Committee of Science,in the frame of the research project number 18T-1C-329;Funding for the DPAC has been provided by national institutions,in particular the institutions participating in the Gaia Multilateral Agreement;a joint project of the University of California,Los Angeles,and the Jet Propulsion Laboratory/California Institute of Technology,funded by the National Aeronautics and Space Administration;the Pan-STARRS1 Surveys(PS1)and the PS1public science archive;which have been made possible under Grant No.NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate;the National Science Foundation Grant No.AST-1238877。
We present a detailed spectroscopic study of pre-main sequence star V565 Mon,which is the illuminating star of the Parsamian 17 cometary nebula.Observations were performed with the 2.6 m telescope in Byurakan Astrophy...
partly supported by the Bulgarian Ministry of Education and Science under the National Program for Research“Young Scientists and Postdoctoral Students”;partial support by grant DN 18-13/2017 from the Bulgarian National Science Fund。
This paper reports results from the first long-term BV(RI)c photometric CCD observations of three variable pre-main-sequence stars collected during the period from February 2007 to January 2020. The investigated stars...
supported by the RA MES State Committee of Science,in the frame of the research project number 18T-1C-329。
We present an analysis of the optical observations of Herbig Ae/Be(HAeBe)star V1686 Cyg,which is associated with a small isolated star-forming region around HAeBe star BD+40?4124.We observed this star as a part of our...
We report the results of optical spectroscopic monitoring observations of a T Tauri star, V409 Tau. A previous photometric study indicated that this star experienced dimming events due to the obscuration of light from...
supported by the Ministry of Education and Science (the basic part of theState assignment, RK No. AAAA-A17-117030310283-7)and by Act No. 211 of the Government of the Russian Federation, agreement 02.A03.21.0006
In our previous papers we have improved the value of the orbital period of the binary Herbig Be star HD 200775 and showed that the [O I] and Si II 6347 and 6371 ?A emission lines displayed variations which correlate w...
the Italian CNAA and MURST (COFIN) grants;the DST-RFBR project INT/RUS/RFBR/P271;BRICS grant number DST/IMRCD/BRICS/PilotCall1/ProFCheap/2017(G) for part of the present work
Using long-term optical, ultraviolet(UV) and X-ray data, we present a study of a classical T Tauri star CV Cha. The V-band light curve obtained from the All Sky Automated Survey(ASAS) shows short as well as long-term ...