Dense filaments are believed to be representative of the initial conditions of star formation in molecular clouds. We have used the MIRI instrument on JWST to image the massive filament NGC 6334M at d ∼ 1.3 kpc with unprecedented resolution and dynamic ...
Philippe André +6 more
doaj +1 more source
Relative Velocities between 13CO Structures within 12CO Molecular Clouds
Velocity fields of molecular clouds (MCs) can provide crucial information on the merger and split between clouds, as well as their internal kinematics and maintenance, energy injection and redistribution, and even star formation within clouds.
Lixia Yuan +12 more
doaj +1 more source
We present the first detection of helium radio recombination lines (HeRRLs) at 800 MHz from the diffuse ionized gas (DIG) in the Cygnus X region, with an ionized helium-to-hydrogen ratio ( ${{n}}_{{\rm{H}}{\rm{e}}}^{+}/{{n}}_{{\rm{H}}}^{+}$ ) of 0.06 ± 0.
D. Anish Roshi +6 more
doaj +1 more source
Formation of S-Bearing Complex Organic Molecules in Interstellar Clouds via Ice Reactions with C2H2, HS, and Atomic H. [PDF]
Santos JC +4 more
europepmc +1 more source
State-of-the-Art Thermochemical and Kinetic Computations for Astrochemical Complex Organic Molecules: Formamide Formation in Cold Interstellar Clouds as a Case Study. [PDF]
Vazart F +4 more
europepmc +1 more source
Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
europepmc +1 more source
Chemiionization in Interstellar Clouds
A. Dalgarno, M. Oppenheimer, R. S. Berry
openaire +1 more source
Increased and varied radiation during the Sun's encounters with cold clouds in the last 10 million years. [PDF]
Opher M +9 more
europepmc +1 more source
TMC-1: Probing the Onset of Chemical Complexity in Space. [PDF]
Agúndez M, Cernicharo J.
europepmc +1 more source
Non-equilibrium preparation of (<i>E</i>)-phosphinimine (HPNH, X<sup>1</sup>A') - a precursor to prebiotic phosphorylating agents. [PDF]
Wang J +8 more
europepmc +1 more source

