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20012024
most citedThe disk-outflow system in the S255IR area of high mass star formation

62 citations · 271 across the 9 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2024

A study of the star clusters' population in the giant molecular cloud G174+2.5

T. A. Permyakova, G. Carraro, A. F. Seleznev +3

We study the structure, interstellar absorption, color-magnitude diagrams, kinematics, and dynamical state of embedded star clusters in the star-forming region associated with the…

astro-ph.GA2019★ 3 cited

RadioAstron probes the ultra-fine spatial structure in the HO maser emission in the star forming region W49N

N. N. Shakhvorostova, A. M. Sobolev, J. M. Moran +3

HO maser emission associated with the massive star formation region W49N were observed with the Space-VLBI mission RadioAstron. The procedure for processing of the maser spectr…

astro-ph.GA2018★ 19 cited

Sun-Sized Water Vapor Masers in Cepheus A

A. M. Sobolev, J. M. Moran, M. D. Gray +6

We present the first VLBI observations of a Galactic water maser (in Chepeus A) made with a very long baseline interferometric array involving the RadioAstron Earth-orbiting satell…

astro-ph.GA2015★ 62 cited

The disk-outflow system in the S255IR area of high mass star formation

I. Zinchenko, S. -Y. Liu, Y. -N. Su +7

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 th…

astro-ph.GA2014★ 14 cited

Distance and proper motion measurement of water masers in Shapless 269 IRS 2w

Yoshiharu Asaki, Hiroshi Imai, Andrej Mikhailovich Sobolev +1

We present astrometric analysis of archival data of water masers in the star-forming region Sharpless 269 (S269) IRS 2w, observed with the VLBI Exploration of Radio Astrometry. An…

astro-ph.GA2012★ 44 cited

The simulation of molecular clouds formation in the Milky Way

S. A. Khoperskov, E. O. Vasiliev, A. M. Sobolev +1

Using 3D hydrodynamic calculations we simulate formation of molecular clouds in the Galaxy. The simulations take into account molecular hydrogen chemical kinetics, cooling and heat…