Leucocytozoon majoris

We present cross-identification of archived X-ray point sources with W UMa variable stars found in the All-Sky Automated Survey… (More)

We observed the midand far-infrared spectral energy distributions of 9 A-type stars from the 300 Myrs old Ursae Majoris group… (More)

ACCRETION disks play an important role in many astrophysical environments, such as active galactic nuclei, protostellar systems… (More)

SU Ursae Majoris systems are short-period binary dwarf novae characterized by two distinct classes of outbursts: ‘normal… (More)

BE Ursae Majoris is a 15-mag variable star of period 2.29 days, with a sinusoidal light curve of ∼1 mag amplitude1. Recently… (More)