Spitzer IRS Spectroscopy of Intermediate Polars: Constraints on Mid-Infrared Cyclotron Emission
arXiv:astro-ph/0611026 · doi:10.1086/510551
Abstract
We present Spitzer Infrared Spectrograph (IRS) observations of eleven intermediate polars (IPs). Spectra covering the wavelength range from 5.2 to 14 m are presented for all eleven objects, and longer wavelength spectra are presented for three objects (AE Aqr, EX Hya, and V1223 Sgr). We also present new, moderate resolution (R 2000) near-infrared spectra for five of the program objects. We find that, in general, the mid-infrared spectra are consistent with simple power laws that extend from the optical into the mid-infrared. There is no evidence for discrete cyclotron emission features in the near- or mid-infrared spectra for any of the IPs investigated. If cyclotron emission is occurring in the 5.2 to 14.0 m bandpass it constitutes less than 1% of the bolometric luminosity of any of the IPs. We discuss our results in the context of the standard model for IPs.
43 pages, including 17 figures, accepted by the Astrophysical Journal
References in corpus (1)
Cited by in corpus (4)
- The Mid-Infrared Spectrum of the Short Orbital Period Polar EF Eridani from the Spitzer Space Telescope
- Abundance Derivations for the Secondary Stars in Cataclysmic Variables from Near-Infrared Spectroscopy
- On the area of accretion curtains from fast aperiodic time variability of the intermediate polar EX Hya
- Near-infrared spectroscopy of 20 new Chandra sources in the Norma Arm