Zobrazeno 1 - 10
of 32
pro vyhledávání: '"Salii, S. V."'
We present results of a spectral survey towards a dense molecular condensation and young stellar objects (YSOs) projected on the border of the HII region RCW 120 and discuss emission of 20 molecules which produce the brightest lines. The survey was p
Externí odkaz:
http://arxiv.org/abs/2403.12934
We study molecular emission in a massive condensation at the border of the HII region RCW 120, paying particular attention to the Core 1 and Core 2 objects, the most massive fragments of the condensation found previously by ALMA. The latter fragment
Externí odkaz:
http://arxiv.org/abs/2102.09145
Autor:
Kirsanova, M. S., Pavlyuchenkov, Ya N., Wiebe, D. S., Boley, P. A., Salii, S. V., Kalenskii, S. V., Sobolev, A. M., Anderson, L. D
The H II region RCW120 is a well-known object, which is often considered as a target to verify theoretical models of gas and dust dynamics in the interstellar medium. However, the exact geometry of RCW120 is still a matter of debate. In this work, we
Externí odkaz:
http://arxiv.org/abs/1908.05394
Publikováno v:
ISSN 1063-7729, Astronomy Reports, 2018, Vol. 62, No. 5, pp. 326-345
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
Externí odkaz:
http://arxiv.org/abs/1805.02465
Autor:
Kirsanova, M. S., Salii, S. V., Sobolev, A. M., Olofsson, A. O. H., Ladeyschikov, D. A., Thomasson, M.
Publikováno v:
Open Astronomy. 26(1): 99-105 (2017). Retrieved 21 Dec. 2017
We studied the distribution of dense gas in a filamentary molecular cloud containing several dense clumps. The center of the filament is given by the dense clump WB673. The clumps are high-mass and intermediate-mass star-forming regions. We observed
Externí odkaz:
http://arxiv.org/abs/1711.01428
Autor:
Zinchenko, I., Liu, S. -Y., Su, Y. -N., Salii, S. V., Sobolev, A. M., Zemlyanukha, P., Beuther, H., Ojha, D. K., Samal, M. R., Wang, Y.
We report the results of our observations of the S255IR area with the SMA at 1.3 mm in the very extended configuration and at 0.8 mm in the compact configuration as well as with the IRAM-30m at 0.8 mm. The best achieved angular resolution is about 0.
Externí odkaz:
http://arxiv.org/abs/1507.05642
Akademický článek
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Autor:
Sutton, E. C., Sobolev, A. M., Salii, S. V., Malyshev, A. V., Ostrovskii, A. B., Zinchenko, I. I.
Publikováno v:
Astrophys.J.609:231-242,2004
We present the results of an interferometric study of 38 millimeter-wave lines of CH3OH in the region around the water maser source W3(H2O) and a region extending about 30" to the south and west of the hydroxyl maser source W3(OH). The methanol emitt
Externí odkaz:
http://arxiv.org/abs/astro-ph/0404412
Autor:
Cragg, D. M., Sobolev, A. M., Ellingsen, S. P., Caswell, J. L., Godfrey, P. D., Salii, S. V., Dodson, R. G.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 323 (2001) 939
We have used the ATNF Mopra antenna and the SEST antenna to search in the directions of several class II methanol maser sources for emission from six methanol transitions in the frequency range 85-115 GHz. The transitions were selected from excitatio
Externí odkaz:
http://arxiv.org/abs/astro-ph/0101311
We obtained rotation temperatures and column densities of methanol CH3OH and propine CH3CCH towards Herbig Ae/Be star V645 Cyg using rotation diagrams. С использованием метода вращательных диаграмм были п
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______917::3b18f77281d6b971b05af0c7ba65352a
https://hdl.handle.net/10995/116123
https://hdl.handle.net/10995/116123