Zobrazeno 1 - 9
of 9
pro vyhledávání: '"O. L. Ryabukhina"'
Autor:
O. L. Ryabukhina, Maria S. Kirsanova
Publikováno v:
Astronomy Reports. 64:394-405
We report observations of molecular line emission toward dense clumps of the WB 673 interstellar filament: WB 668, WB 673, S233–IR, and G173.57+2.43. The observations were done with the 20-m telescope at the Onsala Space Observatory (Sweden). Maps
We present observations of ammonia emission lines toward the interstellar filament WB~673 hosting the dense clumps WB~673, WB~668, S233-IR and G173.57+2.43. LTE analysis of the lines allows us to estimate gas kinetic temperature ($\lesssim$ 30~K in a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8cbefdb4f9e9f19917219d0c6e9dbb20
Autor:
Igor Zinchenko, O. L. Ryabukhina
We present results of a multi-line study of the filamentary infrared dark cloud G351.78-0.54 in the 1.3 and 0.8 mm wavelength bands. The lines of the three isotopologues of carbon monoxide CO, N$_2$H$^+$, CH$_3$CCH and HNCO were observed. The aim was
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4b0dd27ac27c54717a2c3ed7759bf7b8
http://arxiv.org/abs/2105.03133
http://arxiv.org/abs/2105.03133
Autor:
M. S. Kirsanova, O. L. Ryabukhina
Publikováno v:
Астрономия и исследование космического пространства: Всероссийская с международным участием научная конференция студентов и молодых ученых, посвященная памяти Полины Евгеньевны Захаровой.
We study the molecular filament WB 673 which is located at a distance of 1.8 kpc in the giant molecular cloud G174 + 2.5. Observations of ammonia radiolines NH3 (1,1), (2,2) and (3,3) were carried out in 2019 at the Effelsberg observatory (Germany).
Autor:
M. S. Kirsanova, O. L. Ryabukhina
Publikováno v:
Proceedings of the 48-th International student's conferences "Physics of Space".
Autor:
L. E. Pirogov, O. L. Ryabukhina
Publikováno v:
Proceedings of the 48-th International student's conferences "Physics of Space".
Publikováno v:
Astron. Rep.
Astronomy Reports
Astronomy Reports
The results of a detailed analysis of SMA, VLA, and IRAM observations of the region of massive star formation S255N in CO(2---1), \nh, \nhh, \co and some other lines is presented. Combining interferometer and single-dish data has enabled a more detai
Publikováno v:
Астрономия-2018. Том 1.
Autor:
Manash R. Samal, P. M. Zemlyanukha, Igor Zinchenko, Andrej M. Sobolev, Dmitry A. Ladeyschikov, Christian Henkel, Devendra K. Ojha, O. L. Ryabukhina
Publikováno v:
NASA Astrophysics Data System
Res. Astron. Astrophys.
Research in Astronomy and Astrophysics
Res. Astron. Astrophys.
Research in Astronomy and Astrophysics
We present results of a high resolution study of the filamentary infrared dark cloud G192.76+00.10 in the S254-S258 OB complex in several molecular species tracing different physical conditions. These include three isotopologues of carbon monoxide (C
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c71d2898f690c8006ffbe23d753575db
https://ui.adsabs.harvard.edu/#abs/2018arXiv180208030R
https://ui.adsabs.harvard.edu/#abs/2018arXiv180208030R