VLBA astrometry of the AeBe star EC 95 in Serpens

Details VLBA astrometry of the AeBe star EC 95 in Serpens VLBA astrometry of the AeBe star EC 95 in Serpens

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..231d&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Astrometry, Binaries: General, Magnetic Fields, Radiation Mechanisms: Non-Thermal, Radio Continuum: Stars, Techniques: Interferometric

Scientific paper

We present an analysis of eleven VLBA observation of the binary system EC 95 covering a total observing time span of 2.5 years. Both sources in the system were detected a sufficient number of times to allow for high quality independent astrometric fits. The trigonometric parallax obtained from these fits corresponds to a distance d = 429±2 pc. Our observations further suggest that both components in EC 95 could be young stellar objects of intermediate mass.

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