output
19932026
Showing 2014Show all

185 papers · 1 filter

astro-ph.EP2014★ 230 cited

The Mass of Kepler-93b and The Composition of Terrestrial Planets

Courtney D. Dressing, David Charbonneau, Xavier Dumusque +32

Kepler-93b is a 1.478 +/- 0.019 Earth radius planet with a 4.7 day period around a bright (V=10.2), astroseismically-characterized host star with a mass of 0.911+/-0.033 solar mass…

astro-ph.SR2014★ 29 cited

The JCMT Gould Belt Survey: Evidence for radiative heating in Serpens MWC 297 and its influence on local star formation

D. Rumble, J. Hatchell, R. A. Gutermuth +61

We present SCUBA-2 450micron and 850micron observations of the Serpens MWC 297 region, part of the JCMT Gould Belt Survey of nearby star-forming regions. Simulations suggest that r…

astro-ph.SR2014★ 14 cited

Herschel imaging of the dust in the Helix Nebula (NGC 7293)

G. C. Van de Steene, P. A. M. van Hoof, K. M. Exter +19

In our series of papers presenting the Herschel imaging of evolved planetary nebulae, we present images of the dust distribution in the Helix nebula (NGC 7293). Images at 70, 160,…

astro-ph.SR2014★ 12 cited

The SiO outflow from IRAS 17233-3603 at high resolution

P. D. Klaassen, K. G. Johnston, S. Leurini +1

Context: Jets and outflows are key ingredients in the formation of stars across the mass spectrum. In clustered regions, understanding powering sources and outflow components poses…

astro-ph.EP2014★ 100 cited

Characterizing K2 Planet Discoveries: A super-Earth transiting the bright K-dwarf HIP 116454

Andrew Vanderburg, Benjamin T. Montet, John Asher Johnson +43

We report the first planet discovery from the two-wheeled Kepler (K2) mission: HIP 116454 b. The host star HIP 116454 is a bright (V = 10.1, K = 8.0) K1-dwarf with high proper moti…

astro-ph.CO2014★ 32 cited

The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3

A. Durkalec, O. Le Fèvre, S. de la Torre +45

The relation between the galaxy stellar mass M_star and the dark matter halo mass M_h gives important information on the efficiency in forming stars and assembling stellar mass in…