activity
20102024
most citedThe Gaia mission

7.1k citations · 11.9k across the 12 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2016★ 84 cited

Gaia Data Release 1 - The Cepheid & RR Lyrae star pipeline and its application to the south ecliptic pole region

G. Clementini, V. Ripepi, S. Leccia +24

We present an overview of the Specific Objects Study (SOS) pipeline developed within the Coordination Unit 7 (CU7) of the Gaia Data Processing and Analysis Consortium (DPAC), the c…

astro-ph.SR2014★ 37 cited

An interferometric study of the post-AGB binary 89 Herculis. II Radiative transfer models of the circumbinary disk

M. Hillen, J. Menu, H. Van Winckel +6

The presence of disks and outflows is widespread among post-AGB binaries. In the first paper of this series, a surprisingly large fraction of optical light was found to be resolved…

astro-ph.SR2010★ 38 cited

Silicon in the dust formation zone of IRC +10216 as observed with PACS and SPIRE on board Herschel

L. Decin, J. Cernicharo, M. J. Barlow +36

The interstellar medium is enriched primarily by matter ejected from evolved low and intermediate mass stars. The outflows from these stars create a circumstellar envelope in which…

astro-ph.SR2010★ 35 cited

The β Pictoris disk imaged by Herschel PACS and SPIRE

B. Vandenbussche, B. Sibthorpe, B. Acke +40

We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V star β Pic. The disk is well resolved in the PACS filters at 70, 100, and 160 μ…

astro-ph.SR2010★ 45 cited

The detached dust shells of AQ And, U Ant, and TT Cyg

F. Kerschbaum, D. Ladjal, R. Ottensamer +14

Detached circumstellar dust shells are detected around three carbon variables using Herschel-PACS. Two of them are already known on the basis of their thermal CO emission and two a…

astro-ph.SR2010★ 42 cited

Herschel PACS and SPIRE imaging of CW Leo

D. Ladjal, M. J. Barlow, M. A. T. Groenewegen +25

Herschel PACS and SPIRE images have been obtained over a 30'x30' area around the well-known carbon star CW Leo (IRC +10 216). An extended structure is found in an incomplete arc of…