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Methods to Classify Cytoplasmic Foci as Mammalian Stress Granules
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三つの古典的なセフェイド変数星は,天の川の核膨らみにある

Noriyuki Matsunaga1, Takahiro Kawadu, Shogo Nishiyama

  • 1Kiso Observatory, Institute of Astronomy, University of Tokyo, 10762-30 Mitake, Kiso-machi, Kiso-gun, Nagano 397-0101, Japan. matsunaga@ioa.s.u-tokyo.ac.jp

Nature
|August 26, 2011
PubMed
まとめ

銀河系の中核の膨らみで星が形成されるのは,エピソード的に起こった. 最近の星形成の爆発は,古典的なセフェイド変数によって示され,約2500万年前の活動を示唆しています.

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