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IR Compendium: Fomalhaut |
Like many other bright stars, Fomalhaut shows evidence of a Vega-like disk. Observations with ISO show disk structure which has been interpreted as a "clumpy" disk. By combining mid IR imaging and spectroscopy of circumstellar fine structure lines of carbon and oxygen, observers were able to obtain a direct measure of the cooling rate of the circumstellar disk with ISO. To greater constrain planetary formation models, observations were taken with ISO-LWS to determine the composition of dust and ice within the disk. This object is expected to saturate for long exposure times.
| Wavelength (microns) | Flux (Janskys) | Reference |
|---|---|---|
| 1.25 | 627 | Glass, I.S., 1974, MNSSA, 33, 53. |
| 1.62 | 416 | Glass, I.S., 1974, MNSSA, 33, 53. |
| 2.2 | 268 | Glass, I.S., 1974, MNSSA, 33, 53. |
| 3.5 | 120 | Glass, I.S., 1974, MNSSA, 33, 53. |
| 4.8 | 71.50 | Glass, I.S., 1974, MNSSA, 33, 53. |
| 12 | 18.2 | IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986) |
| 25 | 4.81 | IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986) |
| 47 | 5.60 | Harvey et al, 1996, ApJ, 471, 973. |
| 60 | 9.02 | IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986) |
| 95 | 6.7 | Harvey et al, 1996, ApJ, 471, 973. |
| 100 | 11.2 | IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986) |
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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. |
DSS 2nd Generation Red (Search the DSS)
2MASS K band (Search the 2MASS Quicklook Image Server)
ISO-CAM 11.3 microns (Search the ISO archive)
5 degree IRAS 12 micron image centered on Fomalhaut ( Retrieve IRAS images using OASIS)
ISO-CAM 14.9 microns (Search the ISO archive)
24, 70, and 160 micron images from the MIPS instrument on Spitzer as published in Stapelfeldt et al, 2004 ApJS, 154, 458 ( Stapelfeldt et al, 2004, ApJS, 154, 548, or retrieve data using Leopard, AOR ID numbers 6627328,6627072, 6627840,6627584)
5 degree IRAS 100 micron image centered on Fomalhaut ( Retrieve IRAS images using OASIS)
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)
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help@spitzer.caltech.edu http://ssc.spitzer.caltech.edu/documents/compendium/fomalhaut/ This file was last modified on Tue Oct 3 15:56:31 2006. |