activity
20102017
most citedDIGIT survey of far-infrared lines from protoplanetary disks I

124 citations · 845 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2017★ 6 cited

Herschel GASPS spectral observations of T Tauri stars in Taurus: unraveling far-infrared line emission from jets and discs

M. Alonso-Martinez, P. Riviere-Marichalar, G. Meeus +5

At early stages of stellar evolution young stars show powerful jets and/or outflows that interact with protoplanetary discs and their surroundings. Despite the scarce knowledge abo…

astro-ph.EP2014★ 35 cited

Herschel evidence for disk flattening or gas depletion in transitional disks

J. T. Keane, I. Pascucci, C. Espaillat +6

Transitional disks are protoplanetary disks characterized by reduced near- and mid-infrared emission with respect to full disks. This characteristic spectral energy distribution in…

astro-ph.SR2013★ 124 cited

DIGIT survey of far-infrared lines from protoplanetary disks I

D. Fedele, S. Bruderer, E. F. van Dishoeck +10

[abridged] We present far-infrared spectroscopic observations of PMS stars taken with Herschel/PACS as part of the DIGIT key project. The sample includes 22 Herbig AeBe and 8 T Tau…

astro-ph.SR2013★ 50 cited

The 69 micron forsterite band in spectra of protoplanetary disks - Results from the Herschel DIGIT programme

B. Sturm, J. Bouwman, Th. Henning +14

Context: We have analysed Herschel-PACS spectra of 32 circumstellar disks around Herbig Ae/Be and T-Tauri stars obtained within the Herschel key programme DIGIT. In this paper we f…

astro-ph.GA2012★ 21 cited

Kinematics of Ionized Gas at 0.01 AU of TW Hya

M. Goto, A. Carmona, H. Linz +4

We report two-dimensional spectroastrometry of Br gamma emission of TW Hya to study the kinematics of the ionized gas in the star-disk interface region. The spectroastrometry with…

astro-ph.EP2011★ 123 cited

An icy Kuiper-Belt around the young solar-type star HD 181327

J. Lebreton, J. -C. Augereau, W. -F. Thi +18

HD 181327 is a young F5/F6V star belonging to the Beta Pictoris moving group (12 Myr). It harbors an optically thin belt of circumstellar material at 90 AU. We aim to study the dus…