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Multi-wavelength study of the disk around the very low-mass star Par-Lup3-4
N. Huelamo, H. Bouy, C. Pinte +8
Par-Lup3-4 is a very low-mass star (spectral type M5) in the Lupus III star-forming region. The object is underluminous by ~4 mag when compared to objects of similar mass in the sa…
Gas in Protoplanetary Discs (GASPS) 1. First results
G. S. Mathews, W. R. F. Dent, J. P. Williams +50
Context - Circumstellar discs are ubiquitous around young stars, but rapidly dissipate their gas and dust on timescales of a few Myr. The Herschel space observatory allows for the…
Where is the warm H2 ? A search for H2 emission from disks around Herbig Ae/Be stars
C. Martin-Zaidi, J-. C. Augereau, F. Menard +4
Mid-IR emission lines of H2 are useful probes to determine the mass of warm gas present in the surface layers of disks. Numerous observations of Herbig Ae/Be stars (HAeBes) have be…
The large-scale disk fraction of brown dwarfs in the Taurus cloud as measured with Spitzer
J. -L. Monin, S. Guieu, C. Pinte +14
Aims. The brown dwarf (BD) formation process has not yet been completely understood. To shed more light on the differences and similarities between star and BD formation processes,…
Continuum and line modelling of discs around young stars. I. 300000 disc models for Herschel/GASPS
Peter Woitke, Christophe Pinte, Ian Tilling +5
We have combined the thermo-chemical disc code ProDiMo with the Monte Carlo radiative transfer code MCFOST to calculate a grid of ~300000 circumstellar disc models, systematically…