activity
19932010
most citedShock Excited Maser Emission from the Supernova Remnant W28

114 citations · 508 across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.GA2010★ 44 cited

Search for Class I methanol masers in low-mass star formation regions

S. V. Kalenskii, L. E. B. Johansson, P. Bergman +4

A survey of young bipolar outflows in regions of low-to-intermediate-mass star formation has been carried out in two class I methanol maser transitions: 7_0-6_1A+ at 44 GHz and 4_{…

astro-ph2006★ 24 cited

Strong magnetic field in W75N OH maser flare

V. I. Slysh, V. Migenes

A flare of OH maser emission was discovered in W75N in 2000. Its location was determined with the VLBA to be within 110 au from one of the ultracompact H II regions, VLA2. The flar…

astro-ph2006★ 1 cited

High resolution OH maser survey in star forming regions

A. E. Ruiz-Velasco, V. Migenes, V. Slysh +1

We present results of a high resolution survey of OH masers in Galactic Star Forming Regions in order to study the maser emission and establish a list of suitable candidates for hi…

astro-ph2005★ 31 cited

The detection of Class I methanol masers towards regions of low-mass star formation

S. V. Kalenskii, V. G. Promyslov, V. I. Slysh +2

Six young bipolar outflows in regions of low-to-intermediate-mass star formation were observed in the 7_0-6_1A+, 8_0-7_1A+, and 5_{-1}-4_0E methanol lines at 44, 95, and 84 GHz, re…

astro-ph2005★ 19 cited

The brightest OH maser in the sky: a flare of emission in W75 N

A. V. Alakoz, V. I. Slysh, M. V. Popov +1

A flare of maser radio emission in the OH-line 1665 MHz has been discovered in the star forming region W75 N in 2003, with the flux density of about 1000 Jy. At the time it was the…

astro-ph2004★ 30 cited

A 4 - 6 GHz Spectral Scan and 8 - 10 GHz Observations of the Dark Cloud TMC-1

S. V. Kalenskii, V. I. Slysh, P. F. Goldsmith +1

The results of the lowest frequency spectral survey carried out toward a molecular cloud and sensitive observations at selected frequencies are presented. The entire Arecibo C-band…