We present 8-13 Âµm narrow-band photometry of the peculiar star V838 Mon in 2002 September. Our spectrum is consistent with a simple power-law spectrum, although a spectrum with excess emission between 9 and 12 Âµm provides a better fit.
Revista Mexicana de Astronomia y Astrofisica
- Pub Date:
- April 2006
- infrared: stars -- stars: individual (V838 Monocerotis)