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Vol. 20 No. 1 (2004)
,
Contributions
Vol. 20 No. 1 (2004)
Contributions
Time-resolved Spectroscopy of Q Cyg
Kafka S.
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−
Tappert C.
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Honeycutt R. K.
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Bianchini A.
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Kafka S.
Astronomy Department, Indiana University, 319 Swain Hall West, Bloomington, IN 47405, USA
Tappert C.
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Honeycutt R. K.
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Bianchini A.
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0000-0001-6466-5771
PDF
PDF
Keywords
H II regions
ISM: Jets and outflows
Stars: Mass loss
Stars: Pre-main sequence
How to Cite
Time-resolved Spectroscopy of Q Cyg. (2004).
Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias
,
20
(1), 237-237.
https://astronomia.unam.mx/journals/rmxac/article/view/2004rmxac..20..237k
hola
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Abstract
A time-resolved optical spectroscopic study of the long-period (P=10.08h) old nova Q Cyg has revealed persistent yet erratic absorption features indicating the presence of a wind, while the system was rising to one of its stunded outbursts.
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