Oxygen abundance distributions in six late-type galaxies based on SALT spectra of H?II regions 4030, NGC 4123, and NGC 4517
A were observed with the South African Large Telescope (SALT). In all 34 H
Aperiodic optical variability of intermediate polars-cataclysmic variables with truncated accretion disksRevnivtsev M.,
Burenin R.,
Bikmaev I.,
Kniazev A.,
Buckley D.,
Pretorius M.,
Khamitov I.,
Ak T.,
Eker Z.,
Melnikov S.,
Crawford S.,
Pavlinsky M. be well described by
a model based on fluctuations propagating in
a truncated accretion disk. The power
Aperiodic optical variability of intermediate polars-cataclysmic variables with truncated accretion disksRevnivtsev M.,
Burenin R.,
Bikmaev I.,
Kniazev A.,
Buckley D.,
Pretorius M.,
Khamitov I.,
Ak T.,
Eker Z.,
Melnikov S.,
Crawford S.,
Pavlinsky M. be well described by
a model based on fluctuations propagating in
a truncated accretion disk. The power
Oxygen abundance distributions in six late-type galaxies based on SALT spectra of H?II regions 4030, NGC 4123, and NGC 4517
A were observed with the South African Large Telescope (SALT). In all 34 H
New luminous blue variable candidates in the NGC 247 galaxy the Local Group. Here we present
a study of two bright Hα sources in the NGC 247 galaxy. Object j004703
SALT observations of the supernova remnant MCSNR J0127−7332 and its associated Be X-ray binary SXP 1062 in the SMC−7332 is the result of supernova explosion within
a bubble produced by the stellar wind of the supernova progenitor
Семейные суды в Канаде, and special ones such as Family Justice Counselors. There is
a tendency to make UFCs act as special hubs