output
20032009
most citedDust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

1.1k citations

Showing 2009Show all

22 papers · 1 filter

astro-ph.EP200934 cited

On fitting planetary systems in counter-revolving configurations

Julie Gayon-Markt, Eric Bois

In Gayon & Bois (2008) and Gayon etal (2009), (i) we studied the theoretical feasibility and efficiency of retrograde mean motion resonances (i.e. two planets are both in orbital r…

astro-ph.SR200920 cited

Imaging the Solar Tachocline by Time-Distance Helioseismology

Junwei Zhao, Thomas Hartlep, A. G. Kosovichev +1

The solar tachocline at the bottom of the convection zone is an important region for the dynamics of the Sun and the solar dynamo. In this region, the sound speed inferred by globa…

astro-ph.EP2009100 cited

Global circulation as the main source of cloud activity on Titan

Sébastien Rodriguez, Stéphane Le Mouélic, Pascal Rannou +11

Clouds on Titan result from the condensation of methane and ethane and, as on other planets, are primarily structured by circulation of the atmosphere. At present, cloud activity m…

astro-ph.GA20091 cited

A New Analysis of the O VI Emitting Nebula around KPD 0005+5106

Ravi Sankrit, W. Van Dyke Dixon

We present observations of O VI 1032 emission around the helium white dwarf KPD 0005+5106 obtained with the Far Ultraviolet Spectroscopic Explorer. Previously published data, repro…

astro-ph.SR2009381 cited

The 0.8-14.5 micron Spectra of Mid-L to Mid-T Dwarfs: Diagnostics of Effective Temperature, Grain Sedimentation, Gas Transport, and Surface Gravity

D. C. Stephens, S. K. Leggett, Michael C. Cushing +6

We present new 5.2-14.5 micron low-resolution spectra of 14 mid-L to mid-T dwarfs, as well as 3.0-4.1 micron spectra for five of these dwarfs. These data are supplemented by existi…

astro-ph.GA200919 cited

Hubble Space Telescope NICMOS Polarization Observations of Three Edge-on Massive YSOs

Janet P. Simpson, Michael G. Burton, Sean W. J. Colgan +4

Massive young stellar objects (YSOs), like low-mass YSOs, appear to be surrounded by optically thick envelopes and/or disks and have regions, often bipolar, that are seen in polari…