Zobrazeno 1 - 10
of 45
pro vyhledávání: '"Sobolev, Andrej M"'
Autor:
Vorster, Jakobus M., Chibueze, James O., Hirota, Tomoya, MacLeod, Gordon C., van der Walt, Johan D., Vorobyov, Eduard I., Sobolev, Andrej M., Juvela, Mika
Publikováno v:
A&A 691, A157 (2024)
HMYSOs gain most of their mass in short bursts of accretion. Maser emission is an invaluable tool in discovering and probing accretion bursts. We observed the 22 GHz water maser response induced by the accretion burst in NGC6334I-MM1B and identified
Externí odkaz:
http://arxiv.org/abs/2408.15700
Autor:
Salii, Svetlana V., Zinchenko, Igor I., Liu, Sheng-Yuan, Sobolev, Andrej M., Aberfelds, Artis, Su, Yu-Nung
We present results of the investigations of the properties of the methanol $J_1 - J_0$ A$^{-+}$ line series motivated by the recent serendipitous detection of the maser emission in the $14_1 - 14_0$ A$^{-+}$ line at 349~GHz in S255IR-SMA1 soon after
Externí odkaz:
http://arxiv.org/abs/2203.09150
Autor:
Yang, Wenjin, Xu, Ye, Choi, Yoon Kyung, Ellingsen, Simon P., Sobolev, Andrej M., Chen, Xi, Li, Jingjing, Lu, Dengrong
We report a simultaneous 44 and 95 GHz class I methanol maser survey toward 144 sources from the 95 GHz class I methanol maser catalog. The observations were made with the three telescopes of the Korean very long baseline interferometry network opera
Externí odkaz:
http://arxiv.org/abs/2005.00392
Autor:
Burns, Ross A., Handa, Toshihiro, Omodaka, Toshihiro, Sobolev, Andrej M., Kirsanova, Maria S., Nagayama, Takumi, Chibueze, James O., Kohno, Mikito, Nakano, Makoto, Sunada, Kazuyoshi, Ladeyschikov, Dmitry A.
Star formation is thought to be driven by two groups of mechanisms; spontaneous collapse and triggered collapse. Triggered star formation mechanisms further diverge into cloud-cloud collision (CCC), "collect and collapse" (C\&C) and shock induced col
Externí odkaz:
http://arxiv.org/abs/1908.00954
We present estimates of brightness temperature for 5 galactic masers in star-forming regions detected at space baselines. Very compact features with angular sizes of about 23-60 micro arcsec were detected in these regions with corresponding linear si
Externí odkaz:
http://arxiv.org/abs/1802.05120
Autor:
Nakashima, Jun-ichi, Ladeyschikov, Dmitry A., Sobolev, Andrej M., Zhang, Yong, Hsia, Chih-Hao, Yung, Bosco H. K.
We report the results of a wide field CO mapping in the region of IRAS 19312+1950. This IRAS object exhibits SiO/H$_2$O/OH maser emission, and is embedded in a chemically-rich molecular component, of which the origin is still unknown. In order to rev
Externí odkaz:
http://arxiv.org/abs/1604.07170
Autor:
Nakashima, Jun-ichi, Sobolev, Andrej M., Salii, Svetlana V., Zhang, Yong, Yung, Bosco H. K., Deguchi, Shuji
We report the result of a systematic methanol observation toward IRAS 19312+1950. The properties of the SiO, H2O and OH masers of this object are consistent with those of mass-losing evolved stars, but some other properties are difficult to explain i
Externí odkaz:
http://arxiv.org/abs/1506.06551
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Kirsanova, Maria S., Wiebe, Dmitry S., Sobolev, Andrej M., Henkel, Christian, Tsivilev, Alexander P.
Gas density and temperature in star forming regions around Sh2-235 are derived from ammonia line observations. This information is used to evaluate formation scenarios and to determine evolutionary stages of the young embedded clusters S235 East1, S2
Externí odkaz:
http://arxiv.org/abs/1310.6123
Autor:
Kirsanova Maria S., Salii Svetlana V., Sobolev Andrej M., Olofsson Anders Olof Henrik, Ladeyschikov Dmitry A., Thomasson Magnus
Publikováno v:
Open Astronomy, Vol 26, Iss 1, Pp 99-105 (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 starforming regions. We observed C
Externí odkaz:
https://doaj.org/article/9552c9c4a17a406b97c9045fc49005f7
