ISAAC M-band spectroscopy of dust embedded sources at the Galactic Center

Details ISAAC M-band spectroscopy of dust embedded sources at the Galactic Center ISAAC M-band spectroscopy of dust embedded sources at the Galactic Center

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jphcs..54...57m&link_type=abstract

"Journal of Physics: Conference Series, Volume 54, Proceedings of "The Universe Under the Microscope - Astrophysics at High Angu

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present our most recent observations in the M-band, ranging from 4.4 to 5.1 micron, of the central parsec of the Galaxy, obtained with the ISAAC spectrograph of the VLT. These observations resulted in unprecedented high quality spectra of the brightest sources of the central parsec which allow us to analyse the spatial distribution, locally and along the line of sight, of the solid and gaseous phase of the CO molecule.

Affiliated with

Also associated with

No associations

Rating

ISAAC M-band spectroscopy of dust embedded sources at the Galactic Center does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with ISAAC M-band spectroscopy of dust embedded sources at the Galactic Center, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ISAAC M-band spectroscopy of dust embedded sources at the Galactic Center will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1547969