Understanding the chemical evolution of young (high-mass) star-forming regions is a central
topic in star formation research. Chemistry is employed as a unique tool 1) to investigate the …

Context. Massive stars form within dense clumps inside giant molecular clouds (GMCs).
Finding appropriate chemical tracers of the dense gas (n (H 2)> several 10 4 cm− 3 or AV> 8 …

ABSTRACT The Bolocam Galactic Plane Survey (BGPS) is a 1.1 mm continuum survey of
dense clumps of dust throughout the Galaxy covering 170 deg 2. We present spectroscopic …

Abstract We present 12 CO, 13 CO, and C 18 O data as the next major release for the
CHaMP project, an unbiased sample of Galactic molecular clouds in l= 280–300. From a …

ABSTRACT The Census of High-and Medium-mass Protostars (CHaMP) is the first large-
scale (280< l< 300,− 4< b< 2), unbiased, subparsec resolution survey of Galactic molecular …

Abstract We present Stratospheric Observatory For Infrared Astronomy (SOFIA)+ Atacama
Large Millimeter/submillimeter Array (ALMA) continuum and spectral-line polarization data …

We used far-infrared (FIR) and sub-millimetre continuum data from Herschel and the
Atacama Pathfinder EXperiment (APEX) to fit pixel-by-pixel modified Planck spectral energy …

We report the second complete molecular line data release from the Census of High-and
Medium-mass Protostars (CHaMP), a large-scale, unbiased, uniform map** survey at sub …

The results of spectral observations in the GHz frequency range of six objects in the
southern sky containing dense cores and associated with regions of formation of massive …

We obtained continuum maps at a wavelength of 350 μm for eight gas–dust clouds from the
southern hemisphere using the APEX-12m telescope. The clouds are related to the regions …