Výsledky vyhledávání - "星間物質"

Observation of north-east region of supernova remnant RCW86 by Suzaku

Autor: Yamaguchi, Hiroya

Publikováno v: 宇宙圏研究会高エネルギー宇宙物理連絡会,第8回研究会集録原稿:超新星とその残骸 = Proceedings of the 8th Workshop of High Energy AstroPhysics Association, Workshop for Space Astrophysics: Supernova and Its Remnant. :93-97

本収録ではSuzaku(すざく: ASTRO-E2: X-ray Astronomy Satellite)によるRCW86北東shellの観測結果を報告する。イメージングおよびスペクトル解析によって、この領域からのX線を低温(〜0.3keV)および高温

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::d726efd8d1b2bbeb93009e9171c3cf0f
http://id.nii.ac.jp/1696/00038426/

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SN1987A after explosion

Autor: Ito, Masayuki

資料番号: AA0063722005

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::f560c452026be715c6eb9028f28aab85
http://id.nii.ac.jp/1696/00038428/

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Transformation due to railgun impact with pseudo-interstellar matter

Autor: Kaneko, Takeo, Kobayashi, Kensei, Yamori, Akira

Publikováno v: スペース・プラズマ研究会平成15年度 = Space Plasma Conference FY2003. :100-103

資料番号: AA0047901024

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::9fa089a4ab085f4ebbf97509c73eb23c
http://id.nii.ac.jp/1696/00012735/

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A study of rapid expanding H(sub 2) region RCW 89

Autor: Brinkmann, W., Yatsu, Yoichi, Kawai, Nobuyuki, Kataoka, Jun

In this paper, we present a study of the expanding H2 region RCW 89 which is thought to be a part of the radio supernova remnant MSH 15-52 and its associated young 150 ms pulsar B1509-58. We had measured the proper motion of each of the plasma clouds

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::c07931ff186ad936e67e699af2224c7a
http://id.nii.ac.jp/1696/00038427/

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Effects of physical characteristics of samples on the shock-wave induced reactions of organic compounds

Autor: Murae, Tatsushi, Iemura, Ikumi, Yamori, Akira

Publikováno v: スペース・プラズマ研究会平成16年度 = Space Plasma Conference FY2004. :43-45

資料番号: AA0063347012

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::95e27e74c880325f5e07711ae516fc33
http://id.nii.ac.jp/1696/00012687/

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X-ray Observation of the Galactic Center

Autor: YAMAUCHI, Shigeo, KOYAMA, Katsuji

Publikováno v: 宇宙科学研究所報告. 特集: 宇宙観測研究報告. 25:215-221

「ぎんが」衛星による銀河中心の観測は, 2種類の方法で行われた。ひとつは月による掩蔽を利用した観測で, もうひとつは6.7keVの鉄輝線マッピングによる観測である。これらの観測で, 銀

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::249352004bbb5121e7dace5e01365688
http://id.nii.ac.jp/1696/00033073/

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Proceedings of the 8th Workshop of High Energy AstroPhysics Association, Workshop for Space Astrophysics: Supernova and its remnant

Autor: High Energy AstroPhysics Association, Institute of Space and Astronautical Science Japan Aerospace Exploration Agency

宇宙圏研究会高エネルギー宇宙物理連絡会,研究会高エネルギー宇宙物理連絡会 20071017-20071019 東京日本
Workshop of High Energy AstroPhysics Association, Workshop for Space Astrophysics High Energy Astrophysic

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::7a854259e37454766f0d824b4d939fcd
http://id.nii.ac.jp/1696/00038423/

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Cometary dust modeling with aggregates consisting of submicron grains

Autor: Kimura, Hiroshi, Chigai, Takeshi, Yamamoto, Tetsuo

Publikováno v: 第38回月・惑星シンポジウム = Proceedings of the 38th ISAS Lunar and Planetary Symposium. :123-123

We model cometary dust by taking into account its formation and evolution. Light scattering, absorption, and emission properties of the dust expected from our model are compared with observations. We assume unprocessed cometary dust as primordial int

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::2dac9a81f21821c13e36a7be596f8c81
http://id.nii.ac.jp/1696/00020542/

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