Computer Science – Performance
Scientific paper
May 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983esoc...17...29l&link_type=abstract
IN: Workshop on ESO's Very Large Telescope, Cargese, Corse, France, May 16-19, 1983, Proceedings (A84-48051 23-89). Garching, We
Computer Science
Performance
Interstellar Matter, Space Observations (From Earth), Telescopes, Charge Coupled Devices, Focal Plane Devices, Galactic Structure, H Ii Regions, Interstellar Gas, Signal To Noise Ratios, Spectrometers
Scientific paper
The Very Large Telescope being planned by the European Southern Observatory offers important possibilities for the study of interstellar matter and extended objects. Attention is given to the nature and prospective performance levels of such focal plane array instruments as hole and slit spectrometers, imaging Fourier Transfer and Fabry-Perot spectrometers, integral field spectrometers, CCDs, photon counters, and electronographic cameras. These will be used in the study of such line emission phenomena as H II regions, loops, SNRs, comets, galactic jets and coronae, and gas in galactic clusters. Continuum emission sources will encompass reflection nebulae, galaxy outer structures, and the diffuse emission surrounding QSOs.
No associations
LandOfFree
The use of a VLT for studying interstellar matter and extended objects 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 The use of a VLT for studying interstellar matter and extended objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The use of a VLT for studying interstellar matter and extended objects will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1585715