Our research focuses on the stellar content of two star-forming regions. The first one is the molecular cloud which includes G45.12+0.13 and G45.07+0.13 UCHII regions around IRAS 19111+1048 and 19110+1045 sources, respectively. Based on infrared photometric data, we identified a rich stellar population, which includes 909 YSOs with different evolutionary stages. Among selected YSOs there are ZAMS objects. The second one is an elongated molecular cloud, which includes IRAS 05184+3635, 05177+3636, 05168+3634, 05162+3639, and 05156+3643 sources. We identified 1224 candidates of YSOs in the molecular cloud with different evolutionary stages. Selected YSOs are mostly younger then 0.1Myr. The distribution of selected YSOs in both star-forming regions shows that there are dense clusters in the vicinity of all IRAS sources.
oai:arar.sci.am:296261
ՀՀ ԳԱԱ Հիմնարար գիտական գրադարան
Aug 1, 2024
Jan 7, 2022
23
https://arar.sci.am/publication/323270
Հրատարակութեան անունը | Թուական |
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Azatyan, N., Stellar population in two star-forming regions | Aug 1, 2024 |
Nikoghosyan, E. Azatyan, N. Harutyunian, H. Baghdasaryan, D. Andreasyan, D.
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Ю. Л. Вартанян Գլխավոր խմբ․՝ Վ․ Հ․ Համբարձումյան (1965-1987) Լ․ Վ․ Միրզոյան (1988-1999) Դ․ Մ․ Սեդրակյան (2000-2017) Ա․ Գ․ Նիկողոսյան (2018-)
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Azatyan, N. M. Nikoghosyan, E. H.