output
19942026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2009Show all

66 papers · 1 filter

astro-ph.CO2009★ 76 cited

The SPECFIND V2.0 catalogue of radio cross-identifications and spectra. SPECFIND meets the Virtual Observatory

B. Vollmer, B. Gassmann, S. Derriere +6

The new release of the SPECFIND radio cross-identification catalogue, SPECFIND V2.0, is presented. It contains 107488 cross-identified objects with at least three radio sources obs…

astro-ph.HE2009★ 2 cited

Radio lobes and X-ray hot spots of the extraordinary microquasar in NGC 7793

Roberto Soria, Manfred Pakull, Jess Broderick +2

We have studied the newly-discovered microquasar in NGC 7793 in radio, optical and X-ray bands. This system comprises a large (250 x 120 pc) line-emitting optical nebula, detected…

astro-ph.CO2009★ 27 cited

The dusty, albeit ultraviolet bright infancy of galaxies

J. Devriendt, C. Rimes, C. Pichon +11

The largest galaxies acquire their mass early on, when the Universe is still youthful. Cold streams violently feed these young galaxies a vast amount of fresh gas, resulting in ver…

astro-ph.GA2009★ 27 cited

Current data on the globular cluster Palomar 14 are not inconsistent with MOND

Gianfranco Gentile, Benoit Famaey, Garry W. Angus +1

Certain types of globular clusters have the very important property that the predictions for their kinematics in the Newtonian and modified Newtonian dynamics (MOND) contexts are d…

astro-ph.SR2009★ 293 cited

The Taurus Spitzer Survey: New Candidate Taurus Members Selected Using Sensitive Mid-Infrared Photometry

L. M. Rebull, D. L. Padgett, C. -E. McCabe +31

We report on the properties of pre-main-sequence objects in the Taurus molecular clouds as observed in 7 mid- and far-infrared bands with the Spitzer Space Telescope. There are 215…

astro-ph.SR2009

Intermediate Mass Stars <--> Massive Stars. A workshop around causes and consequences of differing evolutionary paths

Eric Josselin, Ariane Lançon

The post-main sequence evolution of stars of intermediate or large masses is notoriously complex. In the recent past, a number of workshops and meetings have focused on either the…