activity
19992010
most citedHerschel/HIFI observations of interstellar OH+ and H2O+ towards W49N: a probe of diffuse clouds with a small molecular fraction

171 citations · 619 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2010★ 20 cited

The methanol lines and hot core of OMC2-FIR4, an intermediate-mass protostar, with Herschel-HIFI

M. Kama, C. Dominik, S. Maret +61

In contrast with numerous studies on the physical and chemical structure of low- and high-mass protostars, much less is known about their intermediate-mass counterparts, a class of…

astro-ph.GA2010★ 20 cited

The origin of the [C II] emission in the S140 PDRs - new insights from HIFI

C. Dedes, M. Röllig, B. Mookerjea +38

Using Herschel's HIFI instrument we have observed [C II] along a cut through S140 and high-J transitions of CO and HCO+ at two positions on the cut, corresponding to the externally…

astro-ph.SR2010★ 20 cited

Discovery of water vapour in the carbon star V Cygni from observations with Herschel/HIFI

D. A. Neufeld, E. González-Alfonso, G. Melnick +25

We report the discovery of water vapour toward the carbon star V Cygni. We have used Herschel's HIFI instrument, in dual beam switch mode, to observe the 1(11) - 0(00) para-water t…

astro-ph.GA2010★ 171 cited

Herschel/HIFI observations of interstellar OH+ and H2O+ towards W49N: a probe of diffuse clouds with a small molecular fraction

D. A. Neufeld, J. R. Goicoechea, P. Sonnentrucker +50

We report the detection of absorption by interstellar hydroxyl cations and water cations, along the sight-line to the bright continuum source W49N. We have used Herschel's HIFI ins…

astro-ph2006★ 35 cited

The high velocity outflow in NGC6334I

S. Leurini, P. Schilke, B. Parise +3

We observed the high velocity outflow originating from NGC6334I in several CO transitions with the APEX telescope, with the goal of deriving the physical parameters of the gas. Usi…

astro-ph2006★ 40 cited

First observations with CONDOR, a 1.5 THz heterodyne receiver

M. C. Wiedner, G. Wieching, F. Bielau +15

The THz atmospheric windows centered at roughly 1.3 and 1.5~THz, contain numerous spectral lines of astronomical importance, including three high-J CO lines, the N+ line at 205 mic…