We present the results of the investigation of ISM and the young stellar population in the IRAS 18316-0602 star-forming region which is referred to as UCHII (G25.65+1.05). Single temperature modified blackbody model shows that values of N(H2) hydrogen column density and Td dust temperature are in ranges 2 - 7x1023 cm-2 and 12 - 30 K, respectively. The analysis of infrared photometric data allowed to reveal about 50 young stellar objects in the G25.65+1.05 UCHII region.
oai:arar.sci.am:296378
ՀՀ ԳԱԱ Հիմնարար գիտական գրադարան
Aug 1, 2024
Jan 7, 2022
15
https://arar.sci.am/publication/323311
Edition name | Date |
---|---|
Andreasyan, D., Infrared study of IRAS 18316-0602 star-forming region | Aug 1, 2024 |
Nikoghosyan, E. Azatyan, N. Harutyunian, H. Baghdasaryan, D. Andreasyan, D.
Azatyan, N. Nikoghosyan, E. Harutyunian, H. Baghdasaryan D. Andreasyan, D.
Harutyunian, H. A. Nikoghosyan, E. H. Azatyan, N. M.
Nikoghosyan, E. H. Harutyunian, H. A. Azatyan, N. M. Grigoryan, A. M.
Azatyan, N. Nikoghosyan, E. Kaper, L. Andreasyan, D. Samsonyan, A. Yeghikyan, A. Baghdasaryan, D. Harutyunyan, N.
Ю. Л. Вартанян Գլխավոր խմբ․՝ Վ․ Հ․ Համբարձումյան (1965-1987) Լ․ Վ․ Միրզոյան (1988-1999) Դ․ Մ․ Սեդրակյան (2000-2017) Ա․ Գ․ Նիկողոսյան (2018-)
Yeghikyan, A. G. Samsonyan, A. L. Harutyunyan, N. A. Azatyan, N. M. Andreasyan, D. H. Baghdasaryan, D. S. Nikoghosyan, E. H.
Azatyan, N. M. Nikoghosyan, E. H.