The detection of infrared emission from the dusty disk around a distant star signals the presence of the H3+ ion. The finding may provide a vital clue to how hydrogen and helium condense into gas-giant planets.
机构:
Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, JapanNASA, GSFC, CRESST II & Xray Astrophys Lab, Greenbelt, MD 20771 USA
Ishida, M.
LIVES AND DEATH-THROES OF MASSIVE STARS,
2017,
12
(S329):
: 361
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361