output
20102025
most citedThe Transiting Circumbinary Planets Kepler-34 and Kepler-35

484 citations

Showing 2012Show all

7 papers · 1 filter

astro-ph.SR2012★ 69 cited

Warm water deuterium fractionation in IRAS 16293-2422 - The high-resolution ALMA and SMA view

Magnus V. Persson, Jes K. Jørgensen, Ewine F. van Dishoeck

Measuring the water deuterium fractionation in the inner warm regions of low-mass protostars has so far been hampered by poor angular resolution obtainable with single-dish ground-…

astro-ph.SR2012★ 36 cited

Strong irradiation of protostellar cores in Corona Australis

J. E. Lindberg, J. K. Jørgensen

The importance of the physical environment in the evolution of newly formed low-mass stars remains an open question. In particular, radiation from nearby more massive stars may aff…

astro-ph.SR2012★ 73 cited

Fundamental properties of the Population II fiducial stars HD 122563 and Gmb 1830 from CHARA interferometric observations

O. L. Creevey, F. Thévenin, T. S. Boyajian +17

We have determined the angular diameters of two metal-poor stars, HD 122563 and Gmb 1830, using CHARA and Palomar Testbed Interferometer observations. For the giant star HD 122563,…

astro-ph.EP2012★ 78 cited

The Transiting System GJ1214: High-Precision Defocused Transit Observations and a Search for Evidence of Transit Timing Variation

K. B. W. Harpsøe, S. Hardis, T. C. Hinse +37

Aims: We present 11 high-precision photometric transit observations of the transiting super-Earth planet GJ1214b. Combining these data with observations from other authors, we inve…

astro-ph.EP2012★ 484 cited

The Transiting Circumbinary Planets Kepler-34 and Kepler-35

William F. Welsh, Jerome A. Orosz, Joshua A. Carter +43

Most Sun-like stars in the Galaxy reside in gravitationally-bound pairs of stars called "binary stars". While long anticipated, the existence of a "circumbinary planet" orbiting su…

astro-ph.CO2012★ 11 cited

Halo abundances and shear in void models

David Alonso, Juan García-Bellido, Troels Haugboelle +1

We study the non-linear gravitational collapse of dark matter into halos through numerical N-body simulations of Lemaitre-Tolman-Bondi void models. We extend the halo mass function…