Spectroscopy of a brown dwarf candidate in the Alpha Persei open cluster
Intermediate-resolution spectroscopy in the range 625-775 nm is reported for a faint very-late-type object discovered in two CCD images taken near the center of the Alpha Per cluster. The spectrum shows strong absorption molecular bands, H-alpha emission, and KI absorption typical of late-M dwarfs; H-alpha varies conspicuously. The effective
Rebolo, Rafael et al.
Fecha de publicación:
4
1992