output
19952026
most citedThe supernova rate per unit mass

546 citations

Showing 2011Show all

14 papers · 1 filter

astro-ph.GA2011★ 42 cited

Multiscale magnetic fields in spiral galaxies: evolution and reversals

David Moss, Rodion Stepanov, Tigran Arshakian +3

Magnetic fields in nearby, star-forming galaxies reveal both large-scale patterns and small-scale structures. A large-scale field reversal may exist in the Milky Way but no such re…

astro-ph.GA2011★ 8 cited

GM 2-4 - a signpost for low and intermediate mass star formation

Tigran Khanzadyan, Tigran A. Movsessian, Chris J. Davis +3

We present a multi-wavelength study of the region towards the GM 2-4 nebula and the nearby source IRAS 05373+2340. Our near-infrared H2 1-0 S(1) line observations reveal various sh…

astro-ph.CO2011★ 21 cited

Optical Spectroscopic ATLAS of the MOJAVE/2cm AGN Sample (1)

Janet Torrealba, Vahram Chavushyan, Irene Cruz-González +3

We present an optical spectroscopic atlas at intermediate resolution (8-15A) for 123 core-dominated radio-loud active galactic nuclei with relativistic jets, drawn from the MOJAVE/…

astro-ph.CO2011

Five Supernova Survey Galaxies in the Southern Hemisphere: Supernova Ia Rates

A. A. Hakobyan, A. R. Petrosian, G. A. Mamon +9

Based on the database of 56 supernovae (SNe) events discovered in 3838 galaxies of the southern hemisphere, we compute the rate of SNe of different types along the Hubble sequence…

astro-ph.SR2011★ 33 cited

Young Exoplanet Transit Initiative (YETI)

R. Neuhäuser, R. Errmann, A. Berndt +80

We present the Young Exoplanet Transit Initiative (YETI), in which we use several 0.2 to 2.6m telescopes around the world to monitor continuously young (< 100 Myr), nearby (< 1 kpc…

astro-ph.SR2011★ 6 cited

Revised classification of the SBS carbon star candidates including the discovery of a new emission line dwarf carbon star

C. Rossi, K. S. Gigoyan, M. G. Avtandilyan +1

Faint high latitude carbon stars are rare objects commonly thought to be distant, luminous giants. For this reason they are often used to probe the structure of the Galactic halo;…