activity
20052017
most citedMolecular Line Emission as a Tool for Galaxy Observations (LEGO). I. HCN as a tracer of moderate gas densities in molecular clouds and galaxies

133 citations · 202 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2017★ 133 cited

Molecular Line Emission as a Tool for Galaxy Observations (LEGO). I. HCN as a tracer of moderate gas densities in molecular clouds and galaxies

Jens Kauffmann, Paul F. Goldsmith, Gary Melnick +3

Trends observed in galaxies, such as the Gao \& Solomon relation, suggest a linear relation between the star formation rate and the mass of dense gas available for star formation.…

astro-ph2007

New water masers in Seyfert and FIR bright galaxies. II

P. Castangia, A. Tarchi, C. Henkel +1

Recently, a relationship between the water maser detection rate and far infrared (FIR) flux density has been found as a result of a 22 GHz maser survey in a sample comprised of nor…

astro-ph2006★ 1 cited

Towards a kinematic model of the Local Group

A. Brunthaler, M. J. Reid, H. Falcke +2

Measuring the proper motions and geometric distances of galaxies within the Local Group is very important for our understanding of the history, present state and future of the Loca…

astro-ph2006★ 68 cited

The Proper Motion of the Local Group Galaxy IC 10

A. Brunthaler, M. J. Reid, H. Falcke +2

We have measured the proper motion of the Local Group galaxy IC 10 with the Very Long Baseline Array by measuring the position of an H2O maser relative to two background quasars ov…

astro-ph2006

Ammonia in Infrared Dark Clouds

Thushara Pillai, Friedrich Wyrowski, Sean J. Carey +1

Infrared Dark Clouds appear to be the long sought population of cold and dense aggregations with the potential of harbouring the earliest stages of massive star formation. Up to no…

astro-ph2005

Quasars in the MAMBO blank field survey

Hauke Voss, Frank Bertoldi, Chris Carilli +5

Our MAMBO 1.2 mm blank field imaging survey of ~0.75 sqd has uncovered four unusually bright sources, with flux densities between 10 and 90 mJy, all located in the Abell 2125 field…