Results 81 to 90 of about 4,398 (186)

Theoretical Spectroscopic Study of Isopropyl Alcohol (CH3-CHOH-CH3)

The Astrophysical Journal
Accurate spectroscopic parameters of isopropyl alcohol, a volatile organic compound present on Earth and in extraterrestrial atmospheres, are provided.
Mohammed Salah, Khadija Marakchi, Najia Komiha, Maria Luisa Senent   +3 more
doaj   +1 more source

Why Are MgC₃H Isomers Missing in the Interstellar Medium? [PDF]

J Phys Chem A, 2022
Panda S, Sivadasan D, Job N, Sinjari A, Thirumoorthy K, Anoop A, Thimmakondu VS.   +6 more
europepmc   +1 more source

Preparation of methanediamine (CH₂(NH₂)₂)-A precursor to nucleobases in the interstellar medium. [PDF]

Proc Natl Acad Sci U S A, 2022
Marks JH, Wang J, Fortenberry RC, Kaiser RI.   +3 more
europepmc   +1 more source

Filamentary Hierarchies and Superbubbles: Galactic Multiscale Magnetohydrodynamic Simulations of Giant Molecular Cloud to Star Cluster Formation

The Astrophysical Journal
There is now abundant observational evidence that star formation is a highly dynamical process that connects filament hierarchies and supernova feedback from galaxy-scale kiloparsec filaments and superbubbles to giant molecular clouds (GMCs) on 100 pc ...
Bo Zhao, Ralph E. Pudritz, Rachel Pillsworth, Hector Robinson, James Wadsley   +4 more
doaj   +1 more source

Galactic Cosmic Rays Throughout the Heliosphere and in the Very Local Interstellar Medium. [PDF]

Space Sci Rev, 2022
Rankin JS, Bindi V, Bykov AM, Cummings AC, Della Torre S, Florinski V, Heber B, Potgieter MS, Stone EC, Zhang M.   +9 more
europepmc   +1 more source

Variations of Interstellar Gas-to-dust Ratios at High Galactic Latitudes

The Astrophysical Journal
Interstellar dust at high Galactic latitudes can influence astronomical foreground subtraction, produce diffuse scattered light, and soften the UV spectra of quasars.
J. Michael Shull, Georgia V. Panopoulou
doaj   +1 more source

Physical Properties and H i-to-H2 Transition across Taurus Linear Edge

The Astrophysical Journal
Studying the atomic-to-molecular transition is essential for understanding the evolution of the interstellar medium. The linear edge of the Taurus molecular cloud, clearly identified in the ^13 CO(1–0) intensity map, serves as an ideal site for ...
Ningyu Tang, Feihang Miao, Gan Luo, Di Li, Junzhi Wang, Fujun Du, Donghong Wu, Shu Liu   +7 more
doaj   +1 more source

Survival of polycyclic aromatic hydrocarbon knockout fragments in the interstellar medium. [PDF]

Nat Commun, 2021
Gatchell M, Ameixa J, Ji M, Stockett MH, Simonsson A, Denifl S, Cederquist H, Schmidt HT, Zettergren H.   +8 more
europepmc   +1 more source

The density distribution and 58.4 nm radiation intensity of interstellar helium in the heliosphere: a model simulation

Earth and Planetary Physics
Research on the interstellar medium and its interaction with the solar system constitutes a significant topic in planetary physics. As the Sun traverses the local interstellar cloud, interstellar neutrals penetrate the heliosphere, forming the ...
JiaLing Lyu, ChongJing Yuan, Fei He, BeiLi Ying   +3 more
doaj   +1 more source

The Heliosphere and Local Interstellar Medium from Neutral Atom Observations at Energies Below 10 keV. [PDF]

Space Sci Rev, 2022
Galli A, Baliukin II, Bzowski M, Izmodenov VV, Kornbleuth M, Kucharek H, Möbius E, Opher M, Reisenfeld D, Schwadron NA, Swaczyna P.   +10 more
europepmc   +1 more source