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Updated: May 20, 2026

Bringing the Visible Universe into Focus with Robo-AO
10:35

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Published on: February 12, 2013

茶色矮星以前のインターフェロメトリック識別

Philippe André1, Derek Ward-Thompson, Jane Greaves

  • 1Laboratoire d'Astrophysique, Instrumentation et Modélisation (AIM), Commissariat à l'Energie Atomique (CEA)/Direction des Sciences de la Matière (DSM)-CNRS-Université Paris Diderot, Gif-sur-Yvette, France. philippe.andre@cea.fr

Science (New York, N.Y.)
|July 7, 2012
PubMed
まとめ

研究者らは,茶色矮星の前核を特定し,茶色矮星が星のように形成されるという理論を支持した. このガスと塵の凝縮は,茶色矮星範囲内の質量を持っています.

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