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

1.4k citations

Showing 2015 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2015★ 9 cited

Dichotomy in the population of young AGN: optical, radio and X-ray properties

M. Kunert-Bajraszewska

There are numerous examples of radio sources with various sizes which surprisingly exhibit very similar morphology. This observational fact helped to create a standard evolutionary…

astro-ph.GA2015★ 28 cited

AGN duty cycle estimates for the ultra-steep spectrum radio relic VLSS J1431.8+1331

A. Shulevski, R. Morganti, P. D. Barthel +19

Steep spectrum radio sources associated with active galactic nuclei (AGN) may contain remnants of past AGN activity episodes. Novel instruments like the LOw Frequency ARray (LOFAR)…

astro-ph.GA2015★ 204 cited

Launching cosmic-ray-driven outflows from the magnetized interstellar medium

Philipp Girichidis, Thorsten Naab, Stefanie Walch +10

We present a hydrodynamical simulation of the turbulent, magnetized, supernova (SN)-driven interstellar medium (ISM) in a stratified box that dynamically couples the injection and…

astro-ph.GA2015★ 18 cited

The 6614 diffuse interstellar absorption band: evidence for internal excitation of the carrier

Charlotte C. M. Marshall, Jacek Krełowski, Peter J. Sarre

An analysis of absorption profiles of the 6614 diffuse interstellar band recorded along the lines-of-sight towards HD 179406 (20 Aql) and HD 147889 is described. The difference…

astro-ph.GA2015★ 42 cited

Discovery of four periodic methanol masers and updated light curve for a further one

M. Szymczak, P. Wolak, A. Bartkiewicz

We report the discovery of 6.7 GHz methanol maser periodic flares in four massive star forming regions and the updated light curve for the known periodic source G22.357+0.066. The…

astro-ph.GA2015★ 16 cited

The structure and kinematics of the the Galaxy thin gaseous disc outside the solar orbit

G. A. Galazutdinov, A. Strobel, F. A. Musaev +2

The rotation curve of the Galaxy is generally thought to be flat. However, using radial velocities from interstellar molecular clouds, which is common in rotation curve determinati…