Results 151 to 160 of about 301,064 (245)
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
Dance to Demise—How Massive Stars May Form Dense Circumstellar Shells before Explosion
We investigate the evolution of red supergiant (RSG) progenitors of core-collapse supernovae (SNe) with initial masses between 12 and 20 M _⊙ , focusing on the effects of enhanced mass loss due to pulsation-driven instabilities in their envelopes and ...
Sutirtha Sengupta +2 more
doaj +1 more source
Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source
Unconventional gas-phase preparation of the prototype polycyclic aromatic hydrocarbon naphthalene (C10H8) via the reaction of benzyl (C7H7) and propargyl (C3H3) radicals coupled with hydrogen-atom assisted isomerization. [PDF]
He C +9 more
europepmc +1 more source
Calcium dicarbide, CaC _2 , has been characterized at high resolution in the laboratory, and its main isotopologue, ^40 CaC _2 , has been assigned to 14 rotational emission lines between 14 and 115 GHz, including 12 previously unassigned lines, in the ...
H. Gupta +8 more
doaj +1 more source
The study of aromatic and resonance-stabilized radicals reaction mechanisms has a key importance for understanding the processes of molecular mass growth of polycyclic aromatic hydrocarbons (PAHs) and carbon nanoparticles in various astrophysical ...
V. S. Krasnoukhov +2 more
doaj +1 more source
Disk in the Circumstellar Envelope of Carbon Mira V Cygni
Asymptotic giant branch (AGB) stars are the primary source of dust and complex molecules in the interstellar medium. The determination of outflow parameters is often hindered by the unknown geometry of the circumstellar environment, creating a demand for
Boris S. Safonov +4 more
doaj +1 more source
The Protostars in Orion: Characterizing the Properties of Their Magnetized Envelopes
We present a study connecting the physical properties of protostellar envelopes to the morphology of the envelope-scale magnetic field. We used the Atacama Large Millimeter/submillimeter Array (ALMA) polarization observations of 61 young protostars at 0 ...
Bo Huang +19 more
doaj +1 more source
Investigating Asymmetry Development from SiO to H2O Maser Regions in VX Sagittarii
Simultaneous very-long-baseline interferometry monitoring observations of H _2 O and SiO masers toward VX Sagittarii were conducted from 2014 February to 2019 January.
Dong-Hwan Yoon +4 more
doaj +1 more source
The mystery of unidentified infrared emission bands. [PDF]
Kwok S.
europepmc +1 more source

