activity
20102014
most citedA spectroscopy study of nearby late-type stars, possible members of stellar kinematic groups

132 citations · 705 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2014★ 8 cited

Herschel -PACS observations of [OI] and H2O in Cha II

P. Riviere-Marichalar, A. Bayo, I. Kamp +11

Gas plays a major role in the dynamical evolution of protoplanetary discs. Its coupling with the dust is the key to our understanding planetary formation. Studying the gas content…

astro-ph.SR2014★ 86 cited

Gas and dust in the Beta Pictoris Moving Group as seen by the Herschel Space Observatory

P. Riviere-Marichalar, D. Barrado, B. Montesinos +11

Context. Debris discs are thought to be formed through the collisional grinding of planetesimals, and can be considered as the outcome of planet formation. Understanding the proper…

astro-ph.EP2013★ 76 cited

Herschel's "Cold Debris Disks": Background Galaxies or Quiescent Rims of Planetary Systems?

A. V. Krivov, C. Eiroa, T. Löhne +24

(abridged) Infrared excesses associated with debris disk host stars detected so far peak at wavelengths around ~100μm or shorter. However, six out of 31 excess sources in the Hersc…

astro-ph.SR2011★ 83 cited

Gas modelling in the disc of HD 163296

I. Tilling, P. Woitke, G. Meeus +19

We present detailed model fits to observations of the disc around the Herbig Ae star HD 163296. This well-studied object has an age of ~ 4 Myr, with evidence of a circumstellar dis…

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.SR2010★ 132 cited

A spectroscopy study of nearby late-type stars, possible members of stellar kinematic groups

J. Maldonado, R. M. Martínez-Arnáiz, C. Eiroa +2

Nearby late-type stars are excellent targets for seeking young objects in stellar associations and moving groups. The origin of these structures is still misunderstood, and lists o…