Zobrazeno 1 - 10
of 49
pro vyhledávání: '"Nikoghosyan, E."'
Massive stars are always the focus of astronomical research and a significant part of them (10--20%) moves in space at a high (supersonic) velocity. This paper presents the results of a study of the $\alpha$ Crucis system, located at $\sim$114 pc dis
Externí odkaz:
http://arxiv.org/abs/2407.09934
Autor:
Azatyan, N., Nikoghosyan, E., Samsonyan, A., Elia, D., Kaper, L., Yeghikyan, A., Andreasyan, D., Baghdasaryan, D.
Understanding the characteristics of young stellar populations is essential for deriving insights into star formation processes within parent molecular clouds and the influence of massive stars. This study focuses on YSOs in the G 045.49+00.04 molecu
Externí odkaz:
http://arxiv.org/abs/2406.05091
Publikováno v:
Astrophysics and Space Science, 2021
This study aims to determine the main physical parameters (N(H2) hydrogen column density and Td dust temperature) of the Interstellar medium, and their distribution in the extended star-forming region, which includes IRAS 05156+3643, 05162+3639, 0516
Externí odkaz:
http://arxiv.org/abs/2111.02906
Autor:
Nikoghosyan, E. H.
Publikováno v:
2017CoBAO..64..126N
The technical achievements of our civilization are accompanied by certain negative consequences affect the near-Earth space. The problem of clogging of near-Earth space by "space debris" as purely theoretical arose essentially as soon as the first ar
Externí odkaz:
http://arxiv.org/abs/1812.10478
Publikováno v:
A&A 603, A26 (2017)
Aims. We report the discovery of a strong outburst of the embedded young stellar object (YSO), namely UKIDSS-J185318.36+012454.5, located in the star-forming region associated with IRAS 18507+0121 source and GAL 034.4+00.23 HII region. Methods. Using
Externí odkaz:
http://arxiv.org/abs/1612.09190
The results of a search for compact clusters in the vicinity of 19 IRAS sources based on data from the GPS UKIDSS and Spitzer GLIMPSE surveys are presented. Overall, clusters have been identified in 15 regions. Clusters are identified for the first t
Externí odkaz:
http://arxiv.org/abs/1608.02225
One of the most prominent features of young objects in the optical range is the presence of emission lines, in particular Ha at 6563A. Therefore, Ha emission is the most common spectroscopic means for identifying young stars. We present the search's
Externí odkaz:
http://arxiv.org/abs/1512.02729
Autor:
Azatyan, N. M., Nikoghosyan, E. H.
The results of the searching on the bases of GPS UKIDSS survey's data of dense compact stellar clusters in the vicinity of 20 YSOs with high and middle masses are presented. Totally we have revealed clusters in 13 areas. Around 5 objects (IRAS 18151-
Externí odkaz:
http://arxiv.org/abs/1506.01053
In this work the results of the statistical analysis of the 215 stars with Ha emission in the IC 348 cluster are presented. The sample is completed to R<20.0.The optical radius is about 11 arcmin. The percentage of emission stars increase from bright
Externí odkaz:
http://arxiv.org/abs/1504.01156
Four binary objects and one triplet have been revealed in the young stellar cluster located in the vicinity of IRAS 05137+3919 source on a distance 4.4 kpc with the use of statistic analysis. They are including the pair of AeBe stars. The percentage
Externí odkaz:
http://arxiv.org/abs/1501.06717