The Livermore sodium laser guide-star launched from the Lick 3-m telescope.
This infrared image of NGC 2024 from Leuschner
Observatory was taken with the undergraduate
IR camera. Red corresponds to K-band (2.2 microns), green is H-band
(1.6 microns), and blue is J-band (1.2 microns). NGC 2024 is a region
of massive star formation in the Orion molecular cloud. Heavy foreground
extinction due to interstellar dust reddens many of the stars in this cluster.
Even at 2.2 microns, where the extinction is one tenth of that at visible
wavelengths, prominent dark dust lanes are apparent. The field of view
is 5.7 arc minutes x 5.7 arc minutes. The exposure time is 80 seconds per
filter and the limiting magnitude is ~ 14.2 at J and ~ 13 at K. Construction
of the infrared camera was made possible by funds from the National
Science Foundation and Rockwell International and described by Graham
& Treffers (2001, Pub. Astr. Soc. Pac.,
113, 607) . The data were reduced using computers donated by Sun
Microsystems.
Dr James R. Graham
Professor of Astronomy
601 Campbell
Hall
University of California
Berkeley CA 94720-3411
tel: (510) 642-8283
fax: (510) 642-3411
Last updated March 2006