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IR Compendium:Cha HA 1


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Table of Contents


Basic Information


Cha H Alpha 1 was the first brown dwarf detected in the X-ray (detected with ROSAT). Its status as a brown dwarf has been confirmed by both near IR colors and spectroscopy. This is the only confirmed brown dwarf observed with ISO, and it is tentatively identified as IRAS point source 11058-7721.

Infrared Fluxes

Wavelength (microns) Flux (Janskys) Reference
1.25 7.24e-3 Carpenter et al, 2002, AJ, 124, 1001
1.65 9.55e-3 Carpenter et al, 2002, AJ, 124, 1001
2.22 9.45e-3 Carpenter et al, 2002, AJ, 124, 1001
6.7 6.7e-3 Persi et al, 2000, A&A, 357, 219
12 2.20 IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)
25 3.37 IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)
60 1.55 IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)
100 7.46e+1 IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)

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)

ISO-CAM 6.7 microns (Search the ISO archive)

5 degree IRAS 12 micron image centered on Cha H Alpha 1 ( Retrieve IRAS images using OASIS)

ISO-CAM 14.3 microns (Search the ISO archive)

ISO-PHT 60 microns (Search the ISO archive)

ISO-PHT 80 microns (Search the ISO archive)

5 degree IRAS 100 micron image centered on Cha H Alpha 1 ( Retrieve IRAS images using OASIS)

ISO-PHT 100 microns (Search the ISO archive)

ISO-PHT 150 microns (Search the ISO archive)

Spitzer Observations

Further reading


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

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