関連する実験動画

Updated: Jul 19, 2026

Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
09:38

Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies

Published on: December 18, 2015

候補星間芳香分子による赤外線放射スペクトル

D J Cook1, S Schlemmer, N Balucani

  • 1Department of Chemistry, University of California, Berkeley 94720-1460, USA.

Nature
|March 21, 1996
PubMed
まとめ

ポリサイクル芳香炭化水素 (PAH) は,星形成の鍵です. 実験室のスペクトルは,中性PAHが恒星間赤外線帯にほとんど寄与しないことを示していますが,それらの充電された形態とより大きなPAHは,おそらくの源です.

キーワード:
NASAの規律 エクゾバイオロジーNASAの規範52-10号についてNASA エクゾバイオロジープログラム非NASAのセンターです.

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