The University of Tokyo
The University of Tokyo
The University of Tokyo
Institute of Astronomy, School of Science, The University of Tokyo
Nagoya University
Kobe University
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)
The University of Tokyo
出版者
宇宙航空研究開発機構(JAXA)
出版者（英）
Japan Aerospace Exploration Agency (JAXA)
雑誌名
宇宙航空研究開発機構特別資料
雑誌名(英)
JAXA Special Publication: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life
巻
JAXA-SP-17-009E
ページ
281 - 284
発行年
2018-03-09
会議概要（会議名, 開催地, 会期, 主催者等）
第4回「あかり」国際会議 (2017年10月17-20日. 東京大学), 文京区, 東京
会議概要（会議名, 開催地, 会期, 主催者等）（英）
The 4th AKARI International Conference: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (October 17-20, 2017. The University of Tokyo), Bunkyo-ku, Tokyo, Japan
抄録（英）
The AKARI all sky surveys provide us unique and independent infrared datasets of classical and recurrent novae taken with two photometric bands at 9 micrometers (S9W) and 18 micrometers (L18W) of the Infrared Camera (IRC) and four photometric bands at 65 micrometers (N60), 90 micrometers (WIDE-S), 140 micrometers (WIDE-L) and 160 micrometers (N160) of the Far-infrared Surveyor (FIS). This allows us to systematically examine the temporal evolution of the infrared spectral energy distributions (SEDs) of novae over epochs from 2006 May to 2007 August every six months. We have searched for infrared counter part of 57 targets including classical novae, recurrent novae and dusty CV, which have been observed with multi-wavelengths. In the AKARI IRC/FIS all sky surveys, 3 novae, V445 Pup, RR Tel, and V838 Mon, were detected both in the mid-infrared and far-infrared. Nine other novae, T CrB, DZ Cru, V2361 Cyg, V476 Sct, RS Oph, V2362 Cyg, V1065 Cen, V1280 Sco, and V745 Sco, were detected only in the mid-infrared. We have investigated the properties of infrared emission associated with those targets. In particular, for some objects, the temporal evolution of infrared emissions before and after the dust formation episode in the nova ejecta is discussed.
内容記述
形態: カラー図版あり
内容記述（英）
Physical characteristics: Original contains color illustrations
Properties of Infrared Emission of Novae Detected in AKARI All Sky Survey
AA1730026052.pdf
(204.67KB)
