output
20022009
most citedRestoring the density-gradient expansion for exchange in solids and surfaces

12k citations

Showing 2007 · astro-phShow all

21 papers · 2 filters

astro-ph20076 cited

Helioseismic Ring Analysis of CME Source Regions

S. C. Tripathy, S. de Wet, K. Jain +2

We apply the ring diagram technique to source regions of halo coronal mass ejections (CMEs) to study changes in acoustic mode parameters before, during, and after the onset of CMEs…

astro-ph2007182 cited

XO-3b: A Massive Planet in an Eccentric Orbit Transiting an F5V Star

Christopher M. Johns-Krull, Peter R. McCullough, Christopher J. Burke +13

We report the discovery of a massive (Mpsini = 13.02 +/- 0.64 Mjup; total mass 13.25 +/- 0.64 Mjup), large (1.95 +/- 0.16 Rjup) planet in a transiting, eccentric orbit (e = 0.260 +…

astro-ph200713 cited

Warm Molecular Gas in M51: Mapping the Excitation Temperature and Mass of H_2 with the Spitzer Infrared Spectrograph

G. Brunner, K. Sheth, L. Armus +7

We have mapped the warm molecular gas traced by the H_2 S(0) - H_2 S(5) pure rotational mid-infrared emission lines over a radial strip across the nucleus and disk of M51 (NGC 5194…

astro-ph2007173 cited

The double Subgiant Branch of NGC 1851: the role of the CNO abundance

S. Cassisi, M. Salaris, A. Pietrinferni +4

We explore the possibility that the anomalous split in the Subgiant branch of the galactic globular cluster NGC 1851 is due to the presence of two distinct stellar populations with…

astro-ph200748 cited

Star Spot Induced Radial Velocity Variability in LkCa 19

Marcos Huerta, Christopher M. Johns-Krull, L. Prato +2

We describe a new radial velocity survey of T Tauri stars and present the first results. Our search is motivated by an interest in detecting massive young planets, as well as inves…

astro-ph200753 cited

Characterizing the Near-UV Environment of M Dwarfs

Lucianne M. Walkowicz, Christopher M. Johns-Krull, Suzanne L. Hawley

We report the results of our HST snapshot survey with the ACS HRC PR200L prism, designed to measure the near-UV emission in a sample of nearby M dwarfs. 33 stars were observed, spa…