First 2.2 micrometer results from the IOTA interferometer

Details First 2.2 micrometer results from the IOTA interferometer First 2.2 micrometer results from the IOTA interferometer

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aj....109..378d&link_type=abstract

The Astronomical Journal (ISSN 0004-6256), vol. 109, no. 1669, p. 378-382

Astronomy and Astrophysics

Astronomy

17

Infrared Astronomy, Infrared Imagery, Near Infrared Radiation, Photosphere, Radio Emission, Red Giant Stars, Infrared Telescopes, Michelson Interferometers, Stellar Temperature, Variable Stars

Scientific paper

We present the first infrared fringe visibility measurements made with the Infrared Optical Telescope Array on Mt. Hopkins. Effective temperatures are derived for RX Boo, RS Cnc, and Beta Peg. RX Boo is the coolest small-amplitude variable giant star to have an effective temperature determination. We compare the size of its photosphere at infrared wavelengths with the sizes of its SiO and H20 radio emission regions. We also discuss initial performance parameters for the interferometer.

Affiliated with

Also associated with

No associations

Rating

First 2.2 micrometer results from the IOTA interferometer 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 First 2.2 micrometer results from the IOTA interferometer, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and First 2.2 micrometer results from the IOTA interferometer will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1818364