The Faint SECONDARY to eps Eridani

Details The Faint SECONDARY to eps Eridani The Faint SECONDARY to eps Eridani

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000hst..prop.9247h&link_type=abstract

HST Proposal ID #9247

Physics

Hst Proposal Id #9247 Hot Stars

Scientific paper

In program 8896, we detected a faint point source near eps Eri. In this
program, we will test whether this point source is a true SECONDARY to
eps Eri {same proper motion, late-M - BD spectrum}.

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