activity
20032008
most citedMolecular oxygen in the rho Ophiuchi cloud

142 citations · 193 across the 4 of their papers we have counts for

collaborators

10 papers

astro-ph200828 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-ph200818 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-ph20075 cited

Upper limits to the water abundance in starburst galaxies

C. D. Wilson, R. S. Booth, A. O. H. Oloffson +11

We have searched for emission from the 557 GHz ortho-water line in the interstellar medium of six nearby starburst galaxies. We used the Odin satellite to observe the 1_10-1_01 tra…

astro-ph2007142 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-ph2005

W Hya through the eye of Odin Satellite observations of circumstellar submillimetre HO line emission

K. Justtanont, P. Bergman, B. Larsson +10

We present Odin observations of the AGB star W Hya in the ground-state transition of ortho-H2O, 1(10)-1(01), at 557GHz. The line is clearly of circumstellar origin. Radiative trans…

astro-ph2005

Searching for O in the SMC:Constraints on Oxygen Chemistry at Low Metallicities

C. D. Wilson, A. O. H. Olofsson, L. Pagani +5

We present a 39 h integration with the Odin satellite on the ground-state 118.75 GHz line of O2 towards the region of strongest molecular emission in the Small Magellanic Cloud. Ou…