activity
20002021
most citedWater in star-forming regions with Herschel (WISH): II. Evolution of 557 GHz 110-101 emission in low-mass protostars

273 citations · 6k across the 110 of their papers we have counts for

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Showing 2011Show all

9 papers · 1 filter

astro-ph.SR2011★ 46 cited

The Herschel HIFI water line survey in the low-mass proto-stellar outflow L1448

G. Santangelo, B. Nisini, T. Giannini +8

As part of the WISH (Water In Star-forming regions with Herschel) key project, we report on the observations of several ortho- and para-H2O lines performed with the HIFI instrument…

astro-ph.GA2011★ 36 cited

Water emission from the chemically rich outflow L1157

M. Vasta, C. Codella, A. Lorenzani +7

In the framework of the Herschel-WISH key program, several ortho-H2O and para-H2O emission lines, in the frequency range from 500 to 1700 GHz, were observed with the HIFI instrumen…

astro-ph.SR2011★ 48 cited

Herschel discovery of a new class of cold, faint debris discs

C. Eiroa, J. P. Marshall, A. Mora +25

We present Herschel PACS 100 and 160 micron observations of the solar-type stars alpha Men, HD 88230 and HD 210277, which form part of the FGK stars sample of the Herschel Open Tim…

astro-ph.EP2011★ 55 cited

High precision astrometry mission for the detection and characterization of nearby habitable planetary systems with the Nearby Earth Astrometric Telescope (NEAT)

Fabien Malbet, Alain Léger, Michael Shao +49

(abridged) A complete census of planetary systems around a volume-limited sample of solar-type stars (FGK dwarfs) in the Solar neighborhood with uniform sensitivity down to Earth-m…

astro-ph.GA2011★ 170 cited

Herschel Measurements of Molecular Oxygen in Orion

Paul F. Goldsmith, Rene Liseau, Tom A. Bell +31

We report observations of three rotational transitions of molecular oxygen (O2) in emission from the H2 Peak 1 position of vibrationally excited molecular hydrogen in Orion. We obs…

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…