165 citations · 414 across the 7 of their papers we have counts for
7 papers
Chronos: A NIR spectroscopic galaxy survey. From the formation of galaxies to the peak of activity
I. Ferreras, R. Sharples, J. S. Dunlop +30
Chronos is our response to ESA's call for white papers to define the science for the future L2, L3 missions. Chronos targets the formation and evolution of galaxies, by collecting…
Radial distribution of gas and dust in the two spiral galaxies M99 and M100
M. Pohlen, L. Cortese, M. W. L. Smith +55
By combining Herschel-SPIRE data with archival Spitzer, HI, and CO maps, we investigate the spatial distribution of gas and dust in the two famous grand-design spirals M99 and M100…
Herschel-PACS observation of the 10 Myr old T Tauri disk TW Hya: Constraining the disk gas mass
W. F. Thi, G. Mathews, F. Ménard +49
Planets are formed in disks around young stars. With an age of ~10 Myr, TW Hya is one of the nearest T Tauri stars that is still surrounded by a relatively massive disk. In additio…
The Herschel view of Gas in Protoplanetary Systems (GASPS). First comparisons with a large grid of models
C. Pinte, P. Woitke, F. Menard +49
The Herschel GASPS Key Program is a survey of the gas phase of protoplanetary discs, targeting 240 objects which cover a large range of ages, spectral types, and disc properties. T…
Herschel-SPIRE observations of the disturbed galaxy NGC4438
L. Cortese, G. J. Bendo, A. Boselli +56
We present Herschel-SPIRE observations of the perturbed galaxy NGC4438 in the Virgo cluster. These images reveal the presence of extra-planar dust up to ~4-5 kpc away from the gala…
Mapping the interstellar medium in galaxies with Herschel/SPIRE
S. A. Eales, M. W. L. Smith, C. D. Wilson +57
The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with…
The Herschel Space Observatory view of dust in M81
G. J. Bendo, C. D. Wilson, M. Pohlen +57
We use Herschel Space Observatory data to place observational constraints on the peak and Rayleigh-Jeans slope of dust emission observed at 70-500 microns in the nearby spiral gala…