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Planetary signatures in circumstella...
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Wahhaj, Zahed.
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Planetary signatures in circumstellar debris disks.
紀錄類型:
書目-電子資源 : Monograph/item
正題名/作者:
Planetary signatures in circumstellar debris disks./
作者:
Wahhaj, Zahed.
面頁冊數:
200 p.
附註:
Source: Dissertation Abstracts International, Volume: 66-06, Section: B, page: 3181.
Contained By:
Dissertation Abstracts International66-06B.
標題:
Physics, Astronomy and Astrophysics. -
電子資源:
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3179827
ISBN:
0542200996
Planetary signatures in circumstellar debris disks.
Wahhaj, Zahed.
Planetary signatures in circumstellar debris disks.
- 200 p.
Source: Dissertation Abstracts International, Volume: 66-06, Section: B, page: 3181.
Thesis (Ph.D.)--University of Pennsylvania, 2005.
Keck mid-infrared imaging of circumstellar debris disks around the pre-main sequence stars, beta Pictoris, HR. 4796A and 49 Cet are presented. It is demonstrated that high resolution thermal imaging at mid-infrared wavelengths is the preferred method to resolve the inner regions of circumstellar disks, because of little contamination by the photosphere in this frequency regime. Our maps of the dust morphology reveal features like sharp ring confinement, asymmetric disk brightness, and in the case of beta Pictoris, a multitude of rings with different orbital inclinations. These features join others found in a small but growing number of debris disk discoveries by direct imaging. Taken together, these present a mounting evidence of planetary signatures around pre-main sequence stars. As a first step to understanding star and planet formation in the conditions of specific molecular clouds, the Spitzer Space Telescope photometric measurements of the Chamaeleon II dark clouds are surveyed for young stars with cicumstellar disks. Twenty one new pre-main sequence stars are discovered in the Chamaeleon II dark clouds, identified by Spitzer photometry.
ISBN: 0542200996Subjects--Topical Terms:
1019521
Physics, Astronomy and Astrophysics.
Planetary signatures in circumstellar debris disks.
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Keck mid-infrared imaging of circumstellar debris disks around the pre-main sequence stars, beta Pictoris, HR. 4796A and 49 Cet are presented. It is demonstrated that high resolution thermal imaging at mid-infrared wavelengths is the preferred method to resolve the inner regions of circumstellar disks, because of little contamination by the photosphere in this frequency regime. Our maps of the dust morphology reveal features like sharp ring confinement, asymmetric disk brightness, and in the case of beta Pictoris, a multitude of rings with different orbital inclinations. These features join others found in a small but growing number of debris disk discoveries by direct imaging. Taken together, these present a mounting evidence of planetary signatures around pre-main sequence stars. As a first step to understanding star and planet formation in the conditions of specific molecular clouds, the Spitzer Space Telescope photometric measurements of the Chamaeleon II dark clouds are surveyed for young stars with cicumstellar disks. Twenty one new pre-main sequence stars are discovered in the Chamaeleon II dark clouds, identified by Spitzer photometry.
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