activity
19952007
most citedMolecular oxygen in the rho Ophiuchi cloud

142 citations · 404 across the 9 of their papers we have counts for

collaborators

9 papers

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-ph2003★ 25 cited

Odin observations of H2O in the Galactic Centre

Aa. Sandqvist, P. Bergman, J. Black

The Odin satellite has been used to detect emission and absorption in the 557-GHz H2O line in the Galactic Centre towards the Sgr A* Circumnuclear Disk (CND), and the Sgr A +20 km/…

astro-ph2003★ 28 cited

First detection of NH3 (1,0 - 0,0) from a low mass cloud core: On the low ammonia abundance of the rho Oph A core

R. Liseau, B. Larsson, A. Brandeker +35

Odin has successfully observed the molecular core rho Oph A in the 572.5 GHz rotational ground state line of ammonia, NH3 (J,K = 1,0 - 0,0). The interpretation of this result makes…

astro-ph2003★ 35 cited

First NH3 detection of the Orion Bar

B. Larsson, R. Liseau, P. Bergman +33

Odin has successfully observed three regions in the Orion A cloud, i.e. Ori KL, Ori S and the Orion Bar, in the 572.5 GHz rotational ground state line of ammonia, ortho-NH3 (J,K) =…

astro-ph2002★ 32 cited

Shapes of Molecular Cloud Cores and the Filamentary Mode of Star Formation

Charles L. Curry

Using recent dust continuum data, we generate the intrinsic ellipticity distribution of dense, starless molecular cloud cores. Under the hypothesis that the cores are all either ob…

astro-ph2001★ 24 cited

The Structure and Evolution of Magnetized Cloud Cores in a Zero--Density Background

Charles L. Curry, Steven W. Stahler

Molecular-line observations of star-forming cloud cores indicate that they are not the flattened structures traditionally considered by theory. Rather, they are elongated, perhaps…