L-BAND SPECTROSCOPY WITH MAGELLAN-AO/Clio2: FIRST RESULTS ON YOUNG LOW-MASS COMPANIONS

L-BAND SPECTROSCOPY WITH MAGELLAN-AO/Clio2: FIRST RESULTS ON YOUNG LOW-MASS COMPANIONS

L-band spectroscopy is a powerful probe of cool low-gravity atmospheres: the P, Q, and R branch fundamental transitions of methane near 3.3 mu m provide a sensitive probe of carbon chemistry; cloud thickness modifies the spectral slope across the band; and H-3(+) opacity can be used to detect aurora...

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Bibliographic Details
Main Authors: Stone, Jordan M., Eisner, Josh, Skemer, Andy, Morzinski, Katie M., Close, Laird, Males, Jared, Rodigas, Timothy J., Hinz, Phil, Puglisi, Alfio
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2016
Subjects:
binaries: close
stars: atmospheres
stars: low-mass
Online Access:http://hdl.handle.net/10150/621975
http://arizona.openrepository.com/arizona/handle/10150/621975

Internet

http://hdl.handle.net/10150/621975
http://arizona.openrepository.com/arizona/handle/10150/621975

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