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IR Compendium: V705 Cas


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Table of Contents


Basic Information


Nova Cas 1993 was observed through a ToO program with ISO. From mid IR spectroscopy of novae, one can determine oxygen and neon abundances. Any dust created in a nova event should be visible using IRAC and MIPS.

Infrared Fluxes

Wavelength (microns) Flux (Janskys) Reference
1.25 1.44 Gehrz et al, 1995, ApJ, 448, 119.
1.60 7.37e-1 Gehrz et al, 1995, ApJ, 448, 119.
2.20 1.14e-1 Gehrz et al, 1995, ApJ, 448, 119.
3.80 7.47e-1 Gehrz et al, 1995, ApJ, 448, 119.
4.90 1.42 Gehrz et al, 1995, ApJ, 448, 119.
7.80 6.44 Gehrz et al, 1995, ApJ, 448, 119
8.28 1.891e-1 Egan et al, 1996, AJ, 112, 2862.
9.80 8.43 Gehrz et al, 1995, ApJ, 448, 119.
10.30 8.71 Gehrz et al, 1995, ApJ, 448, 119.

Spectral Energy Distributions



This SED was created using the sensitivity and saturation values available in November 2004. The black dots are the flux values from the above table. The green and red lines are the respective sensitivity and saturation limits for each instrument. The sensitivity values used are for a 5 sigma detection of a point source with a 500 second exposure.

Infrared images

Search SIMBAD for additional data on this object

DSS 2nd Generation Red (Search the DSS)

2MASS K band (Search the 2MASS Quicklook Image Server)

5 degree IRAS 12 micron image centered on V705 Cas ( Retrieve IRAS images using OASIS)

5 degree IRAS 100 micron image centered on V705 Cas ( Retrieve IRAS images using OASIS)

Infrared Spectra

click images for full 2 to 40 micron spectra with ISO-SWS (Search the ISO archive)

click on image for full 40 to 200 micron spectra with ISO-LWS (Search the ISO archive)

Spitzer Observations

Further reading


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This file was last modified on Tue Oct 3 15:56:28 2006.

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