The Peculiarities of the SEI 105 System

Details The Peculiarities of the SEI 105 System The Peculiarities of the SEI 105 System

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jdso....5..177b&link_type=abstract

Journal of Double Star Observations, vol. 5, no. 3, p. 177-179.

Physics

Scientific paper

As described in the previous article, measurement of SEI 105 in the constellation Auriga took place on 12 April 2007. The only measures of this system are from 1895 with parameters of 16.8" and 354 degrees. The present article was written because due to the significant proper motion of the primary star, the angular distance of the main pair has changed, and also because a third member has been measured in our own photos (Figure 1), which has caused no little surprise during its thorough examination.

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