Astronomy and Astrophysics – Astronomy
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.4005s&link_type=abstract
American Astronomical Society Meeting 210, #40.05; Bulletin of the American Astronomical Society, Vol. 39, p.154
Astronomy and Astrophysics
Astronomy
Scientific paper
Transition disks are dusty protoplanetary disks surrounding young stars, where the shape of the thermal-infrared spectral energy distribution indicates a dearth of hot dust that may signify a gap in the inner disk. These objects are thought to represent a very short-lived transitionary phase that may arise either through internal photoevaporation of the inner disk by the central star, or perhaps through clearing of gas and dust in the disk by a young planet. Near the Sun, these objects are extremely rare with only a handful currently known, complicating the task of trying to understand their origin and role in star and planet formation. Here we present the discovery of hundreds of objects in the Carina Nebula that have the spectral signature of these so-called transition disks, with photospheric colors at shorter IR wavelengths, and strong IR excess emission at the longest wavelengths, seen in data obtained during our Spitzer/IRAC survey of the Carina Nebula. We discuss their impact on our view of current star and planet formation in the Carina Nebula, as well as the broader implications for the hypothesis that our own Solar System may have formed alongside very massive stars in a region much like Carina.
Alexander Romannikov
Babler Brian
Bally John
Churchwell Edward
Indebetouw Remy
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