The 21 cm emission from atomic hydrogen (HI) is one of the most important tracers of the
structure and dynamics of the interstellar medium. Thanks to Galactic rotation, the line is …

ABSTRACT GRB 230812B is a bright and relatively nearby (z= 0.36) long gamma-ray burst
(GRB) that has generated significant interest in the community and has thus been observed …

We present the description and initial results of the TRAPUM (TRAnsients And PUlsars with
MeerKAT) search for pulsars associated with supernova remnants (SNRs), pulsar wind …

Context. Strongly lensed quasars are fundamental sources for cosmology. The Gaia space
mission covers the entire sky with the unprecedented resolution of 0.18 ″in the optical …

We report on a discovery of an X-ray emitting circumstellar material (CSM) knot inside the
synchrotron dominant supernova remnant RX J1713. 7− 3946. This knot was previously …

The existence of particle acceleration in the Milky Way has been established for many
decades via observations of cosmic rays (CRs) up to the knee feature in the PeV energy …

We propose a new method for estimating the distances of molecular clouds traced by CO
line emission. Stars from 2MASS and Gaia EDR3 are selected as on-cloud stars when they …

Knowing the Galactic 3D dust distribution is relevant for understanding many processes in
the interstellar medium and for correcting many astronomical observations for dust …