Spectrophotometry of speckle binary stars

Details Spectrophotometry of speckle binary stars Spectrophotometry of speckle binary stars

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002bsao...53...58a&link_type=abstract

Bulletin of the Special Astrophysical Observatory, Vol. 53, P. 58-77

Astronomy and Astrophysics

Astrophysics

7

Stars: Spectrophotometry: Spectral Energy Distribution, Stars: Binaries: Speckle Binary Stars

Scientific paper

Spectrophotometric observations of 20 speckle interferometric binary stars in the wavelength range 3640-8340 Å, with a resolution of 18 Å, are presented in the form of the measured flux corrected for atmospheric extinction in the units of erg/cm2\cdot s \cdot Å, with no corrections for interstellar reddening. B,V, and R magnitudes, B-V colour indices and entire spectral types are also presented and compared with those of Hipparcos and Tycho catalogues and SIMBAD.

Affiliated with

Also associated with

No associations

Rating

Spectrophotometry of speckle binary stars 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 Spectrophotometry of speckle binary stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectrophotometry of speckle binary stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1893586