Three micron spectroscopy of the galactic centre source IRS 7

Details Three micron spectroscopy of the galactic centre source IRS 7 Three micron spectroscopy of the galactic centre source IRS 7

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...154l...5b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 154, no. 1-2, Jan. 1986, p. L5-L7.

Astronomy and Astrophysics

Astrophysics

100

Astronomical Spectroscopy, Galactic Nuclei, Infrared Spectra, Millimeter Waves, Radio Spectroscopy, Absorption Spectra, Astronomical Models, Interstellar Extinction, Interstellar Matter, Spectral Line Width

Scientific paper

A new three-micron band spectrum of the infrared source IRS 7 in Sagittarius A has been obtained from Mauna Kea, using a cooled grating spectrometer with a revolving power of about 350. The profiles of the two broad absorption features, centered at 3.0 and 3.4 microns, are well-characterized in this spectrum. Of the narrow absorption features previously reported, only that at 3.48 microns is detected. No other narrow absorption features with equivalent widths greater than 0.001 microns are resolved. The spectrum provides a firm basis for models of interstellar grains based on extinction curves in this spectral region.

Affiliated with

Also associated with

No associations

Rating

Three micron spectroscopy of the galactic centre source IRS 7 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 Three micron spectroscopy of the galactic centre source IRS 7, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Three micron spectroscopy of the galactic centre source IRS 7 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1843773