Linearly polarized emission from dust grains and molecular spectroscopy is an effective
probe of the magnetic field topology in the interstellar medium and molecular clouds. The …

Astrophysical gases are commonly multiphase and highly turbulent. In this work, we
investigate the survival and growth of cold gas in such a turbulent, multiphase medium using …

Young stellar associations hold a star formation record that can persist for millions of years,
revealing the progression of star formation long after the dispersal of the natal cloud. To …

Abstract The Taurus-Auriga complex is the prototypical low-mass star-forming region, and
provides a unique testbed of the star formation process, which left observable imprints on …

The mean plane-of-sky magnetic field strength is traditionally obtained from the combination
of polarization and spectroscopic data using the Davis–Chandrasekhar–Fermi (DCF) …

The central regions of cool-core galaxy clusters harbour multiphase gas, with gas
temperatures ranging from to. Feedback from active galactic nuclei jets prevents the gas …

We present the first empirical constraints on the turbulent velocity field of the diffuse
circumgalactic medium around four luminous quasi-stellar objects (QSOs) at z≈ 0.5–1.1 …

Photoionization models frequently assume constant temperature or density within H ii
regions. We investigate this assumption by measuring the detailed temperature and density …

The interstellar medium (ISM) is turbulent over vast scales and in various phases. In this
paper, we study turbulence with different tracers in four nearby star-forming regions: Orion …

It has been shown that the gas velocities within the intracluster medium (ICM) can be
measured by applying the novel XMM–Newton EPIC-pn energy scale calibration, which …