Return to search

Properties of debris disks around stars within 25 parsec of the Sun

<p> Debris disk candidates around nearby stars were detected with the <i> Spitzer Space Telescope</i> using the Multiband Imaging Photometer (MIPS) at 24&mu;m (MIPS24) and 70&mu;m (MIPS70). A survey sample of 978 stars within 25pc of the Sun was observed with MIPS24, with 438 stars solely observed with MIPS70. Candidates were defined as target stars with excess infrared emission above the stellar photospheric emission at both 3&sigma; and 5&sigma; levels. At 24&mu;m, debris disks were identied around 262 stars, yielding a detection frequency of 26.8% at the 3&sigma; level. A detection rate of 22.1% is deduced from 216 stars at the 5&sigma; level. The detection frequency at 24&mu;m shows a decreasing trend with late spectral types. A detection rate of 26.5% is implied by 128 MIPS70 candidates at the 3&sigma; level, and 11.8% is revealed by 57 candidates at the 5&sigma; level. At 70&mu;m, our 3&sigma; and 5&sigma; detections correspond to fractional luminosities of 10<sup>-3.</sup>8 and 10<sup>-3.4</sup>, respectively. Both detection rates increase with later spectral types. </p>

Identiferoai:union.ndltd.org:PROQUEST/oai:pqdtoai.proquest.com:1537816
Date19 June 2013
CreatorsWang, Luqian
PublisherNorthern Arizona University
Source SetsProQuest.com
LanguageEnglish
Detected LanguageEnglish
Typethesis

Page generated in 0.0076 seconds