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Optical and IR Observations of Aql X-1
Published online by Cambridge University Press: 12 April 2016
Abstract
We have obtained optical spectra and IR photometry in an attempt to determine the orbital parameters of the Aql X-1 system. Spectra from the MMT in October 1995 appear to detect the secondary, but are not sufficient to measure the mass function. IR photometry in and out of mini-outburst find K ~ 15.4, and may indicate that the disk contributionat K is modest during the mini-outburst.
- Type
- Part 15. Poster Papers
- Information
- International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 705 - 706
- Copyright
- Copyright © Astronomical Society of the Pacific 1997
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