# A survey of 10-μm silicate emission from dust around young sun-like stars ☆

@article{Gaidos2004ASO,
title={A survey of 10-$\mu$m silicate emission from dust around young sun-like stars ☆},
author={Eric Gaidos and Christopher Duro Koresko},
journal={New Astronomy},
year={2004},
volume={9},
pages={33-42}
}
• Published 22 July 2003
• Physics
• New Astronomy
6 Citations

## Figures and Tables from this paper

Ten Micron Observations of Nearby Young Stars
• Physics, Geology
• 2004
We present new 10 μm photometry of 21 nearby young stars obtained at the Palomar 5 m and at the Keck I 10 m telescopes as part of a program to search for dust in the habitable zone of young stars.
Detection of the inner-debris disk of Vega with CHARA/FLUOR
• Physics, Geology
SPIE Astronomical Telescopes + Instrumentation
• 2006
Using the FLUOR beam-combiner installed at the CHARA Array (Mt. Wilson, CA), we have obtained highprecision visibility measurements of Vega, one of the prototypic debris-disk stars, known to be
Circumstellar material in the Vega inner system revealed by CHARA/FLUOR
• Physics, Geology
• 2006
Context. Only a handful of debris disks have been imaged up to now. Due to the need for high dynamic range and high angular resolution, very little is known about the inner planetary region, where
Hot exozodiacal dust resolved around Vega with IOTA/IONIC
• Physics, Geology
• 2011
Context. Although debris discs have been detected around a significant number of main-sequence stars, only a few of them are known to harbour hot dust in their inner part where terrestrial planets
Where Are the M Dwarf Disks Older Than 10 Million Years?
• Physics, Geology
• 2005
We present 11.7 μm observations of nine late-type dwarfs obtained at the Keck I 10 m telescope in 2002 December and 2003 April. Our targets were selected for their youth or apparent IRAS 12 μm
The Nearest Young Moving Groups
• Physics, Geology
• 2006
The latest results in the research of forming planetary systems have led several authors to compile a sample of candidates for searching for planets in the vicinity of the Sun. Young stellar

## References

SHOWING 1-10 OF 33 REFERENCES
8-13 Micron Spectroscopy of Young Stars
• Physics
• 1998
We present 8-13 μm spectra of 23 young stars acquired with the UKIRT CGS3 spectrometer, including T Tauri, Herbig Ae/Be, and FU Orionis stars. Silicate emission and absorption features can generally
Thermal Infrared Imaging and Spectroscopy of Comet Hale-Bopp (C/1995 O1)
• Physics, Geology
• 2000
We present λ = 3-5 and 8-13 μm images and long-slit spectra of comet Hale-Bopp (C/1995 O1) taken in 1997 February-April, near the time of perihelion passage. In agreement with other infrared
Detection of silicates in the 51 Ophiuchi system
• Physics
• 1993
We have detected a prominent 10 μm silicate emission feature in 51 Oph, a B9.5 Ve star with circumstellar emission. 51 Oph shows the Vega phenomenon, probable disk emission from a main-sequence star.
Observational Constraints on Late Heavy Bombardment Episodes around Young Solar Analogs
Thermal emission from dust is investigated around 36 nearby G and K stars selected as analogs to the young Sun during the period of late heavy bombardment on the Moon (prior to 3.8 Ga). Measurements
Structure in the Dusty Debris around Vega
• Physics, Geology
• 2002
We present images of the Vega system obtained with the IRAM Plateau de Bure interferometer at a 1.3 mm wavelength with submillijansky sensitivity and ~2.″5 resolution (about 20 AU). These
A 25 micron search for Vega-like disks around main-sequence stars with ISO
• Physics, Geology
• 2002
We present an ISO 25 m photometric survey of a sample of 81 nearby main-sequence stars in order to determine the incidence of \warm" dust disks. All stars were detected by ISO. We used an empirical
Incidence and survival of remnant disks around main-sequence stars
• Physics, Geology
• 2001
We present photometric ISO 60 and 170 um measurements, complemented by some IRAS data at 60 ${\mu\textrm{m}}$, of a sample of 84 nearby main-sequence stars of spectral class A, F, G and K in order to
On the Near-Infrared Size of Vega
• Physics, Geology
• 2001
Near-infrared (2.2 μm) long baseline interferometric observations of Vega are presented. The stellar disk of the star has been resolved, and the data have been fitted with a limb-darkened stellar
DISCOVERY OF A SHELL AROUND ALPHA-LYRAE
• Physics
• 1984
IRAS observations of Alpha Lyrae reveal a large infrared excess beyond 12 microns. The excess over an extrapolation of a 10,000 K blackbody is a factor of 1.3 at 25 microns, 7 at 60 microns, and 16
The Silicates in the Disk of beta Pictoris
• Physics, Geology
• 1993
We have obtained intermediate-resolution (R≃50) infrared (2.6-13.5 μm) spectra of the particles in the circumstellar disk of β Pic. The silicate dust feature near 10 μm is broader and contains more