Context. Through observations numerous giant molecular filaments (GMFs) have been
discovered in the Milky Way. Their role in the Galactic star formation and Galaxy-scale …

The latest generation of Galactic Plane surveys is enhancing our ability to study the effects of
galactic environment upon the process of star formation. We present the first data from CO …

Context. The Serpens filament, a prominent elongated structure in a relatively nearby
molecular cloud, is believed to be at an early evolutionary stage, so studying its physical and …

We present new ALMA observations of CO, CN, CS, HCN, and HCO absorption seen
against the bright and compact radio continuum sources of eight galaxies. Combined with …

We present the survey of 12 CO/13 CO/C 18 O (J= 1− 0) toward the California molecular
cloud (CMC) within the region of 161 fdg 75≤ l≤ 167 fdg 75,− 9 fdg 5≤ b≤− 7 fdg 5 using …

We present a new method of calculating distances of molecular clouds in the Galactic plane,
using CO observations and the Gaia DR2 parallax and G-band extinction (AG) …

ABSTRACT We present Atacama Large Millimetre/submillimetre Array observations of the
brightest cluster galaxy Hydra-A, a nearby (z= 0.054) giant elliptical galaxy with powerful …

We present results of cloud catalogs of 12 CO, 13 CO, and C 18 O (J= 1–0) in a section of
the third Galactic quadrant over (195< l< 220,∣ b∣< 5) from the Milky Way Imaging Scroll …

We present observations of the J= 1–0 transition lines of 12 CO, 13 CO, and C 18 O toward
the Galactic region of 153 fdg 60≤ l≤ 156 fdg 50 and 1 fdg 85≤ b≤ 3 fdg 50, using the …

Using the H i self-absorption data from the Five-hundred-meter Aperture Spherical radio
Telescope, we perform a study of the cold atomic gas in the Cygnus X North region. The …