activity
20032017
most citedDetection of interstellar hydrogen peroxide

113 citations · 620 across the 17 of their papers we have counts for

collaborators

16 papers

astro-ph.IM2017★ 85 cited

SEPIA - a new single pixel receiver at the APEX Telescope

V. Belitsky, I. Lapkin, M. Fredrixon +31

Context: We describe the new SEPIA (Swedish-ESO PI Instrument for APEX) receiver, which was designed and built by the Group for Advanced Receiver Development (GARD), at Onsala Spac…

astro-ph.SR2015★ 16 cited

On the accretion process in a high-mass star forming region - A multitransitional THz Herschel-HIFI study of ammonia toward G34.26+0.15

M. Hajigholi, C. M. Persson, E. S. Wirström +8

[Abridged] Our aim is to explore the gas dynamics and the accretion process in the early phase of high-mass star formation. The inward motion of molecular gas in the massive star f…

astro-ph.SR2014★ 30 cited

SiO masers from AGB stars in the vibrationally excited v=1,v=2, and v=3 states

J. -F. Desmurs, V. Bujarrabal, M. Lindqvist +3

The v=1 and v=2 J=1-0 (43 GHz), and v=1 J=2-1 (86 GHz) SiO masers are intense in AGB stars and have been mapped using VLBI showing ring-like distributions. Those of the v=1, v=2 J=…

astro-ph.GA2013★ 3 cited

Physical properties of outflows: Comparing CO and H2O based parameters in Class 0 sources

P. Bjerkeli, R. Liseau, B. Nisini +4

Context. The observed physical properties of outflows from low-mass sources put constraints on possible ejection mechanisms. Historically, these quantities have been derived from C…

astro-ph.GA2012

Preliminary results on SiO v=3 J=1-0 maser emission from AGB stars

J. -F. Desmurs, V. Bujarrabal, M. Lindqvist +3

We present the results of SiO maser observations at 43GHz toward two AGB stars using the VLBA. Our preliminary results on the relative positions of the different J=1-0 SiO masers (…

astro-ph.GA2012★ 31 cited

H2O line mapping at high spatial and spectral resolution - Herschel observations of the VLA1623 outflow

P. Bjerkeli, R. Liseau, B. Larsson +12

Apart from being an important coolant, H2O is known to be a tracer of high-velocity molecular gas. Recent models predict relatively high abundances behind interstellar shockwaves.…