Fukagawa, M.; Murakami, H.; Hirao, T.; Yamashita, T.; Ootsubo, T.; Enya, K.; Nakagawa, T.; Fujiwara, H.; Marshall, J. and White, G.J.
|DOI (Digital Object Identifier) Link:||https://doi.org/10.1063/1.3215814|
|Google Scholar:||Look up in Google Scholar|
We present the early results of mid-infrared (MIR) pointed observations of nearby mainsequence stars with AKARI. Out of 117 AFGKM stars, 7 AF-type stars show the large (>7% of the photospheric level) infrared excesses at 24 µm, in which three sources are newly identified with AKARI.
|Item Type:||Journal Article|
|Copyright Holders:||2010 American Institute of Physics|
|Keywords:||origin and evolution; accretion and accretion disks; main-sequence: early-type stars; astronomical catalogs; atlases; sky surveys; databases; retrieval systems; archives|
|Academic Unit/School:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Tracy Bartlett|
|Date Deposited:||05 Dec 2010 08:53|
|Last Modified:||28 Nov 2016 14:15|
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