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  1. B100 理学部/理学研究科
  2. B100a 雑誌掲載論文
  3. 学術雑誌

Mid- and far-infrared properties of Spitzer Galactic bubbles revealed by the AKARI all-sky surveys

http://hdl.handle.net/2237/25268
06b58c25-de7e-4201-be5a-1da2b92530ba
名前 / ファイル ライセンス アクション
hattori2016.pdf hattori2016.pdf ファイル公開:2017/06/01 (11.0 MB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2016-12-20
タイトル
タイトル Mid- and far-infrared properties of Spitzer Galactic bubbles revealed by the AKARI all-sky surveys
著者 Hattori, Yasuki

× Hattori, Yasuki

WEKO 68364

Hattori, Yasuki

Search repository
Kaneda, Hidehiro

× Kaneda, Hidehiro

WEKO 68365

Kaneda, Hidehiro

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Ishihara, Daisuke

× Ishihara, Daisuke

WEKO 68366

Ishihara, Daisuke

Search repository
Fukui, Yasuo

× Fukui, Yasuo

WEKO 68367

Fukui, Yasuo

Search repository
Torii, Kazufumi

× Torii, Kazufumi

WEKO 68368

Torii, Kazufumi

Search repository
Hanaoka, Misaki

× Hanaoka, Misaki

WEKO 68369

Hanaoka, Misaki

Search repository
Kokusho, Takuma

× Kokusho, Takuma

WEKO 68370

Kokusho, Takuma

Search repository
Kondo, Akino

× Kondo, Akino

WEKO 68371

Kondo, Akino

Search repository
Shichi, Kazuyuki

× Shichi, Kazuyuki

WEKO 68372

Shichi, Kazuyuki

Search repository
Ukai, Sota

× Ukai, Sota

WEKO 68373

Ukai, Sota

Search repository
Yamagishi, Mitsuyoshi

× Yamagishi, Mitsuyoshi

WEKO 68374

Yamagishi, Mitsuyoshi

Search repository
Yamaguchi, Yuta

× Yamaguchi, Yuta

WEKO 68375

Yamaguchi, Yuta

Search repository
権利
権利情報 This is a pre-copyedited, author-produced version of an article accepted for publication in [Publications of the Astronomical Society of Japan] following peer review. The version of record [Publications of the Astronomical Society of Japan. v.68, n.3, 2016, p.37] is available online at: http://doi.org/10.1093/pasj/psw028.
キーワード
主題Scheme Other
主題 infrared: ISM
キーワード
主題Scheme Other
主題 ISM: bubbles
キーワード
主題Scheme Other
主題 stars: formation
キーワード
主題Scheme Other
主題 stars: massive
抄録
内容記述 We have carried out a statistical study on the mid- and far-infrared (IR) properties of Galactic IR bubbles observed by Spitzer. Using the Spitzer 8 μm images, we estimated the radii and covering fractions of their shells, and categorized them into closed, broken, and unclassified bubbles with our data analysis method. Then, using the AKARI all-sky images at wavelengths of 9, 18, 65, 90, 140, and 160 μm, we obtained the spatial distributions and the luminosities of polycyclic aromatic hydrocarbon (PAH), warm, and cold dust components by decomposing six-band spectral energy distributions with model fitting. As a result, 180 sample bubbles show a wide range of total IR luminosities corresponding to the bolometric luminosities of a single B-type star to many O-type stars. For all the bubbles, we investigated relationships between the radius, luminosities, and luminosity ratios, and found that there are overall similarities in the IR properties among the bubbles regardless of their morphological types. In particular, they follow a power-law relation with an index of ∼3 between the total IR luminosity and radius, as expected from the conventional picture of the Strömgren sphere. The exceptions are large broken bubbles; they indicate higher total IR luminosities, lower fractional luminosities of the PAH emission, and dust heating sources located nearer to the shells. We discuss the implications of those differences for a massive star-formation scenario.
内容記述タイプ Abstract
出版者
出版者 Oxford University Press
言語
言語 eng
資源タイプ
資源タイプresource http://purl.org/coar/resource_type/c_6501
タイプ journal article
ISSN
収録物識別子タイプ ISSN
収録物識別子 0004-6264
書誌情報 Publications of the Astronomical Society of Japan

巻 68, 号 3, p. 37-37, 発行日 2016-06
著者版フラグ
値 author
URI
識別子 http://doi.org/10.1093/pasj/psw028
識別子タイプ DOI
URI
識別子 http://hdl.handle.net/2237/25268
識別子タイプ HDL
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