The Rise and Fall of Debris Disks: MIPS Observations of h and chi Persei and the Evolution of Mid-IR Emission from Planet Formation
arXiv:0709.2510 · doi:10.1086/523698
Abstract
We describe Spitzer/MIPS observations of the double cluster, h and Persei, covering a 0.6 square-degree area surrounding the cores of both clusters. The data are combined with IRAC and 2MASS data to investigate 616 sources from 1.25-24 . We use the long-baseline -[24] color to identify two populations with IR excess indicative of circumstellar material: Be stars with 24 excess from optically-thin free free emission and 17 fainter sources (J 14-15) with [24] excess consistent with a circumstellar disk. The frequency of IR excess for the fainter sources increases from 4.5 through 24 . The IR excess is likely due to debris from the planet formation process. The wavelength-dependent behavior is consistent with an inside-out clearing of circumstellar disks. A comparison of the 24 excess population in h and Per sources with results for other clusters shows that 24 emission from debris disks 'rises' from 5 to 10 Myr, peaks at 10-15 Myr, and then 'falls' from 15/20 Myr to 1 Gyr.
arXiv comment48 pages, 15 figures, accepted for publication in The Astrophysical Journal
References in corpus (42)
- Disk Frequencies and Lifetimes in Young Clusters
- Circumstellar Dust Disks in Taurus-Auriga: The Submillimeter Perspective
- The Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 microns Using GLIMPSE Data
- Dust coagulation in protoplanetary disks: a rapid depletion of small grains
- Very Low Mass Stars and Brown Dwarfs in Taurus-Auriga
- Observations of IC348: The Disk Population at 2-3 Million Years
- Debris Disk Evolution Around A Stars
- Hectospec, the MMT's 300 Optical Fiber-Fed Spectrograph
- Debris disks in main sequence binary systems
- Reduction Algorithms for the Multiband Imaging Photometer for Spitzer
- Transience of hot dust around sun-like stars
- The 24 Micron Source Counts in Deep Spitzer Surveys
- IRAC Observations of Taurus Pre-Main Sequence Stars
- Steady-state evolution of debris disks around A stars
- Dust Migration and Morphology in Optically Thin Circumstellar Gas Disks
- Age dependence of the Vega Phenomenon: Theory
- The Age of Beta Pic
- Incidence and survival of remnant disks around main-sequence stars
- Collisional Cascades in Planetesimal Disks II. Embedded Planets
- The Evolutionary Status of Be Stars: Results from a Photometric Study of Southern Open Clusters
- Terrestrial Planet Formation I. The Transition from Oligarchic Growth to Chaotic Growth
- Exploring Terrestrial Planet Formation in the TW Hydrae Association
- Detecting the Dusty Debris of Terrestrial Planet Formation
- The Star Formation History and Mass Function of the Double Cluster h and Chi Persei
- Binarity as a key factor in protoplanetary disk evolution: Spitzer disk census of the eta Chamaeleontis cluster
- A Spitzer Study of Dusty Disks in the Scorpius-Centaurus OB Association
- The age dependence of the Vega phenomenon: Observations
- Dusty Rings: Signposts of Recent Planet Formation
- IR observations of MS 1054-03: Star Formation and its Evolution in Rich Galaxy Clusters
- Spitzer observations of the Orion OB1 association: second generation dust disks at 5-10 Myr
- Spitzer 24 micron Survey of Debris Disks in the Pleiades
- Spatially Resolving the Inner Disk of TW Hya
- Debris Disks in NGC 2547
- The Formation and Evolution of Planetary Systems (FEPS): Discovery of an Unusual Debris System Associated with HD 12039
- Spitzer/IRAC and JHKs Observations of h & chi Persei: Constraints on Protoplanetary Disk and Massive Cluster Evolution at ~ 10^{7} yr
- Radial Distribution of Dust Grains Around HR 4796A
- Ultraviolet Emission Line Ratios of Cataclysmic Variables
- High-Resolution Imaging of the Dust Disk around 49 Ceti
- Dust Distribution in Gas Disks II: Self Induced Ring Formation Through a Clumping Instability
- Are Giant Planets Forming Around HR 4796A?
- Terrestrial Zone Debris Disk Candidates in h and chi Persei
- Discovery of Gas Accretion Onto Stars in 13 Myr old h and chi Persei
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- Formation and Evolution of Planetary Systems (FEPS): Properties of Debris Dust around Solar-type Stars
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- Structure and evolution of debris disks around F-type stars: I. Observations, database and basic evolutionary aspects
- The Stellar Population of h and chi Persei: Cluster Properties, Membership, and the Intrinsic Colors and Temperatures of Stars
- The Transitional Protoplanetary Disk Frequency as a Function of Age: Disk Evolution in the Coronet Cluster, Taurus, and Other 1--8 Myr-old Regions
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- The low level of debris disk activity at the time of the Late Heavy Bombardment: a Spitzer study of Praesepe
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- A young hierarchical triple system harbouring a candidate debris disc
- IPHAS A-type Stars with Mid-IR Excesses in Spitzer Surveys
- Circumstellar Disk Evolution: Constraining Theories of Planet Formation
- Analysis of B and Be Star Populations of the Double Cluster h and chi Persei
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