activity
20032026
most citedProbing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles - II. CO line survey of evolved stars: derivation of mass-loss rate formulae

242 citations · 1.9k across the 47 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2025

Detection of CH3+ in the O-rich planetary nebula NGC 6302

Charmi Bhatt, Jan Cami, Els Peeters +33

Planetary nebulae are sites where ejected stellar material evolves into complex molecules, but the precise physical conditions and chemical routes that govern these processes are u…

astro-ph.GA2015

Gas and dust in the star-forming region rho Oph A: The dust opacity exponent beta and the gas-to-dust mass ratio g2d

R. Liseau, B. Larsson, T. Lunttila +6

We aim at determining the spatial distribution of the gas and dust in star-forming regions and address their relative abundances in quantitative terms. We also examine the dust opa…

astro-ph.GA2014★ 3 cited

Resolving the shocked gas in HH54 with Herschel: CO line mapping at high spatial and spectral resolution

P. Bjerkeli, R. Liseau, C. Brinch +11

The HH54 shock is a Herbig-Haro object, located in the nearby Chamaeleon II cloud. Observed CO line profiles are due to a complex distribution in density, temperature, velocity, an…

astro-ph.GA2012★ 23 cited

Herschel/HIFI observations of red supergiants and yellow hypergiants: I. Molecular inventory

D. Teyssier, G. Quintana-Lacaci, A. P. Marston +17

Red supergiant stars (RSGs) and yellow hypergiant stars (YHGs) are believed to be the high-mass counterparts of stars in the AGB and early post-AGB phases. We study the mass-loss i…

astro-ph.GA2012★ 101 cited

Multi-line detection of O2 toward rho Oph A

R. Liseau, P. F. Goldsmith, B. Larsson +36

Models of pure gas-phase chemistry in well-shielded regions of molecular clouds predict relatively high levels of molecular oxygen, O2, and water, H2O. Contrary to expectation, the…

astro-ph.GA2011★ 30 cited

Herschel observations of the Herbig-Haro objects HH52-54

P. Bjerkeli, R. Liseau, B. Nisini +11

We are aiming at the observational estimation of the relative contribution to the cooling by CO and H2O, as this provides decisive information for the understanding of the oxygen c…