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19932023
most citedMolecular oxygen in the rho Ophiuchi cloud

142 citations · 1.1k across the 35 of their papers we have counts for

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astro-ph2008★ 28 cited

Circumstellar water vapour in M-type AGB stars: Constraints from H2O(1_10 - 1_01) lines obtained with Odin

M. Maercker, F. L. Schoeier, H. Olofsson +8

Aims: Spectrally resolved circumstellar H2O(1_10 - 1_01) lines have been obtained towards three M-type AGB stars using the Odin satellite. This provides additional strong constrain…

astro-ph2008★ 18 cited

Odin observations of the Galactic centre in the 118-GHz band. Upper limit to the O2 abundance

Aa. Sandqvist, B. Larsson, Å. Hjalmarson +6

The Odin satellite has been used to search for the 118.75-GHz line of molecular oxygen (O2)in the Galactic centre. Odin observations were performed towards the Sgr A* circumnuclear…

astro-ph2008★ 99 cited

Circumstellar water vapour in M-type AGB stars: Radiative transfer models, abundances and predictions for HIFI

Matthias Maercker, Fredrik L. Schoeier, Hans Olofsson +2

Aims: By performing a detailed radiative transfer analysis, we determine fractional abundances of circumstellar H2O in the envelopes around six M-type asymptotic giant branch stars…

astro-ph2007★ 142 cited

Molecular oxygen in the rho Ophiuchi cloud

B. Larsson, R. Liseau, L. Pagani +56

Molecular oxygen, O2 has been expected historically to be an abundant component of the chemical species in molecular clouds and, as such, an important coolant of the dense interste…

astro-ph2006★ 27 cited

Revealing the environs of the remarkable southern hot core G327.3-0.6

F. Wyrowski, K. M. Menten, P. Schilke +3

We present a submm study of the massive hot core G327.3-0.6 that constrains its physical parameters and environment. The APEX telescope was used to image CO and N2H+ emission, to o…

astro-ph2006★ 34 cited

Submillimeter spectroscopy of southern hot cores: NGC6334(I) and G327.3-0.6

P. Schilke, C. Comito, S. Thorwirth +5

High-mass star-forming regions are known to have a rich molecular spectrum from many species. Some of the very highly excited lines are emitted from very hot and dense gas close to…