Extended hot dust emission around the earliest massive quiescent galaxy
Ji Z +16 more
europepmc +1 more source
A nearby dark molecular cloud in the Local Bubble revealed via H<sub>2</sub> fluorescence. [PDF]
Burkhart B +22 more
europepmc +1 more source
Isotopic chirality and high-resolution gigahertz and terahertz spectroscopy of <i>trans</i>-2,3-dideutero-oxirane (<i>tc</i>-CHDCHDO). [PDF]
Chen Z +6 more
europepmc +1 more source
Exploring the nature of ISM turbulencein disc galaxies
Galaxy formation is a continuous process that started only a few hundred million yearsafter the Big Bang. The first galaxies were very volatile, with bursts of star formationand disorganised gas motions. However, even as these galaxies evolved to have orderlyrotating gas discs, the gas within the disc, referred to as the interstellar medium (ISM),still
openaire +1 more source
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy. [PDF]
Klaassen P +40 more
europepmc +1 more source
Rate constants for a reactive system of astrophysical interest: a statistical study of CH<sub>2</sub>. [PDF]
González-Lezana T +5 more
europepmc +1 more source
Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn
Fujimoto S +45 more
europepmc +1 more source
Supernova dust destruction in the magnetized turbulent ISM. [PDF]
Kirchschlager F, Mattsson L, Gent FA.
europepmc +1 more source
Strong Gravitational Lensing and Microlensing of Supernovae. [PDF]
Suyu SH +4 more
europepmc +1 more source

