Speckle Interferometry at the Observatorio Astronómico Nacional. III

Details Speckle Interferometry at the Observatorio Astronómico Nacional. III Speckle Interferometry at the Observatorio Astronómico Nacional. III

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxaa..47..211o&link_type=abstract

Revista Mexicana de Astronomía y Astrofísica Vol. 47, pp. 211-217 (2011)

Astronomy and Astrophysics

Astronomy

Binaries: Visual, Stars: Fundamental Parameters, Techniques: High Angular Resolution, Techniques: Interferometric

Scientific paper

We present speckle interferometric measurements of binary stars performed during August of 2010 with the 1.5 m telescope and during November of 2010 with the 2.1 m telescope of the Observatorio Astronómico Nacional at SPM (Mexico). We report here the results of 238 measurements of 225 pairs with a primary limiting magnitude of V = 12.2; 211 of them have separations less than 1''. The mean error in separation is 0.03 arcsec 1.5° in position angle. Some of the position angles were determined with the usual 180° ambiguity.

Affiliated with

Also associated with

No associations

Rating

Speckle Interferometry at the Observatorio Astronómico Nacional. III 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 Speckle Interferometry at the Observatorio Astronómico Nacional. III, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Speckle Interferometry at the Observatorio Astronómico Nacional. III will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1673813