Current Capabilities for High Angular Resolution Imaging in the UV/optical

Details Current Capabilities for High Angular Resolution Imaging in the UV/optical Current Capabilities for High Angular Resolution Imaging in the UV/optical

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...204.2503w&link_type=abstract

American Astronomical Society Meeting 204, #25.03; Bulletin of the American Astronomical Society, Vol. 36, p.691

Astronomy and Astrophysics

Astrophysics

Scientific paper

I shall review techniques for obtaining angular resolutions in excess of the diffraction limit at optical and UV wavelengths. Techniques include spectroscopic and Doppler imaging, Doppler tomography, eclipse timing studies, and reverberation mapping techniques. I will discuss the capabilities and limitations of these methods. I will compare these capabilities to those obtainable from interferometric imaging, and will discuss some of the new vistas on astrophysics opened by such data.

Affiliated with

Also associated with

No associations

Rating

Current Capabilities for High Angular Resolution Imaging in the UV/optical 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 Current Capabilities for High Angular Resolution Imaging in the UV/optical, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Current Capabilities for High Angular Resolution Imaging in the UV/optical will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1170986