output
19952026
most citedTrigonometric Parallaxes of High Mass Star Forming Regions: the Structure and Kinematics of the Milky Way

1.4k citations

Showing 2014 · astro-ph.GAShow all

8 papers · 2 filters

astro-ph.GA2014★ 1 cited

Consistent system of oscillator strengths of A -- X (0, 0) and B -- X (0, 0) bands of CH molecule

T. Weselak, G. A. Galazutdinov, P. Gnaciński +1

Detailed analysis of intensity ratios of unsaturated methylidyne (CH) A--X and B--X bands suggests consistency of the recently published oscillator strengths of A -- X$^{2}Π…

astro-ph.GA2014★ 3 cited

Multi-epoch VLBA observations of radio galaxy 0932+075: is this a compact symmetric object?

A. Marecki, A. Sokołowska

A part of the radio structure of the galaxy 0932+075 emerged as a possible compact symmetric object (CSO) after the observation with the Very Long Baseline Array (VLBA) at 5 GHz in…

astro-ph.GA2014★ 24 cited

Detection of vibronic bands of C in a translucent cloud towards HD 169454

M. R. Schmidt, J. Krełowski, G. A. Galazutdinov +4

We report the detection of eight vibronic bands of C, seven of which have been hitherto unobserved in astrophysical objects, in the translucent cloud towards HD~169454. Four of…

astro-ph.GA2014★ 24 cited

EVN observations of 6.7 GHz methanol masers in clusters of massive young stellar objects

Anna Bartkiewicz, Marian Szymczak, Huib van Langevelde

Methanol masers at 6.7 GHz are associated with high-mass star-forming regions (HMSFRs) and often have mid-infrared (MIR) counterparts characterized by extended emission at 4.5 m…

astro-ph.GA2014★ 66 cited

Flux upper limits for 47 AGN observed with H.E.S.S. in 2004-2011

H. E. S. S. Collaboration, A. Abramowski, F. Aharonian +217

About 40% of the observation time of the High Energy Stereoscopic System (H.E.S.S.) is dedicated to studying active galactic nuclei (AGN), with the aim of increasing the sample of…

astro-ph.GA2014★ 21 cited

6.7GHz methanol maser variability in Cepheus A

M. Szymczak, P. Wolak, A. Bartkiewicz

6.7 GHz methanol maser emission from the well-studied star-forming region Cepheus A was monitored with the Torun 32 m radio telescope. We found synchronized and anticorrelated chan…