High angular resolution in the infrared with a single Very Large Telescope (VLT)

Details High angular resolution in the infrared with a single Very Large Telescope (VLT) High angular resolution in the infrared with a single Very Large Telescope (VLT)

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983esoc...17..163l&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

Astronomy and Astrophysics

Astronomy

Angular Resolution, Infrared Astronomy, Infrared Interferometers, Speckle Patterns, Telescopes, Active Galactic Nuclei, Atmospheric Effects, Signal To Noise Ratios

Scientific paper

Greater angular resolution, better photon collection capability, and superior seeing at the appropriate site, are the advantages anticipated from the application of the European Southern Observatory's Very Large Telescope to IR speckle interferometry. The astrophysical consequences of these performance improvements are greater insight into such star formation processes as stellar winds, disks, mass ejection, fragmentation, Kelvin-Helmholtz instabilities and the role of magnetic fields. It is also anticipated that advancements will be made in the appearance of protoplanetary systems and the structure of IR emission in active galactic nuclei.

Affiliated with

Also associated with

No associations

Rating

High angular resolution in the infrared with a single Very Large Telescope (VLT) 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 High angular resolution in the infrared with a single Very Large Telescope (VLT), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High angular resolution in the infrared with a single Very Large Telescope (VLT) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1585734