We report the discovery of a debris system associated with the 30 Myr old G3/5V star HD 12039 using Spitzer Space Telescope observations from 3.6–160 m. An observed infrared excess (LIR /L 1; 104) above the ex-pected photosphere for k k14 m is fit by thermally emittingmaterial with a color temperature of T 110K, warmer than the majority of debris disks identified to date around Sun-like stars. The object is not detected at 70 mwith a 3 upper limit 6 times the expected photospheric flux. The spectrum of the infrared excess can be explained bywarm, op-tically thinmaterial comprised of blackbody-like grains of sizek7m that reside in a belt orbiting the star at 4–6AU. An alternate model dominated by smaller grains, near the blowout size a ...
We present data obtained with the Infrared Array Camera (IRAC) aboard the Spitzer Space Telescope (S...
Aims. Uncovering the ingredients and the architecture of planetary systems is a very active field of...
As part of a large SpitzerMIPS Guaranteed Time Observation program, we have searched for infrared ex...
We report the discovery of a debris system associated with the ~30 Myr old G3/5V star HD 12039 using...
We report the discovery of a debris system associated with the ~30 Myr old G3/5V star HD 12039 using...
Not Available We report the discovery of a debris system associated with the ~30 Myr old G3/5V star...
We present the discovery of debris systems around three solar mass stars based upon observations per...
We present the discovery of debris systems around three Sun-like stars based on observations perfo...
We present 3-160 micron photometry obtained with the IRAC and MIPS instruments for the first five ta...
We present 3-160 mum photometry obtained with the Infrared Array Camera (IRAC) and Multiband Im...
We present 3-160 mum photometry obtained with IRAC and MIPS, spectrophotometry from 5-35 mum using...
We present Spitzer photometric (IRAC and MIPS) and spectroscopic (IRS low resolution) observations f...
Since giant planets scatter planetesimals within a few tidal radii of their orbits, the locations of...
Aims. Uncovering the ingredients and the architecture of planetary systems is a very active field of...
Dust in debris disks is generated by collisions among planetesimals. The existence of these planetes...
We present data obtained with the Infrared Array Camera (IRAC) aboard the Spitzer Space Telescope (S...
Aims. Uncovering the ingredients and the architecture of planetary systems is a very active field of...
As part of a large SpitzerMIPS Guaranteed Time Observation program, we have searched for infrared ex...
We report the discovery of a debris system associated with the ~30 Myr old G3/5V star HD 12039 using...
We report the discovery of a debris system associated with the ~30 Myr old G3/5V star HD 12039 using...
Not Available We report the discovery of a debris system associated with the ~30 Myr old G3/5V star...
We present the discovery of debris systems around three solar mass stars based upon observations per...
We present the discovery of debris systems around three Sun-like stars based on observations perfo...
We present 3-160 micron photometry obtained with the IRAC and MIPS instruments for the first five ta...
We present 3-160 mum photometry obtained with the Infrared Array Camera (IRAC) and Multiband Im...
We present 3-160 mum photometry obtained with IRAC and MIPS, spectrophotometry from 5-35 mum using...
We present Spitzer photometric (IRAC and MIPS) and spectroscopic (IRS low resolution) observations f...
Since giant planets scatter planetesimals within a few tidal radii of their orbits, the locations of...
Aims. Uncovering the ingredients and the architecture of planetary systems is a very active field of...
Dust in debris disks is generated by collisions among planetesimals. The existence of these planetes...
We present data obtained with the Infrared Array Camera (IRAC) aboard the Spitzer Space Telescope (S...
Aims. Uncovering the ingredients and the architecture of planetary systems is a very active field of...
As part of a large SpitzerMIPS Guaranteed Time Observation program, we have searched for infrared ex...