Results 61 to 70 of about 110,395 (224)
Centrosymmetric molecules as possible carriers of diffuse interstellar bands [PDF]
In this paper, we present new data with interstellar C2 (Phillips bands A-X), from observations made with the Ultraviolet-Visual Echelle Spectrograph of the European Southern Observatory. We have determined the interstellar column densities and excitation temperatures of C2 for nine Galactic lines. For seven of these, C2 has never been observed before,
arxiv +1 more source
The Orientation of the Local Interstellar Magnetic Field
The orientation of the local interstellar magnetic field introduces asymmetries in the heliosphere that affect the location of heliospheric radio emissions and the streaming direction of ions from the termination shock of the solar wind.
Gombosi, T. I., Opher, M., Stone, E. C.
core +1 more source
Solving the Puzzle of the Carbonic Acid Vibrational Spectrum – an Anharmonic Story
The harmonic picture is the basic approximation that allows the prediction of vibrational spectra. However, reality is neither decoupled nor harmonic. This can lead to problems in notation and the assignment of individual bands. Taking anharmonicity and mode coupling into account allows a drastic improvement in spectral clarity.
Jonas Schlagin+5 more
wiley +1 more source
Overtone Transition 2ν1 of HCO+ and HOC+: Origin, Radiative Lifetime, Collisional Quenching
The C−H/O−H stretch vibration overtone of one of the simplest molecular ion isomeric systems HCO+/HOC+ is studied in a cryogenic ion trap experiment. Moreover, our comprehensive “zero background” method enables the determination of radiative lifetimes and select quenching reaction rates at the same time.
Miguel Jiménez‐Redondo+5 more
wiley +1 more source
Using high-resolution UV data obtained from the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope, we focus on eight sight lines along the Sun’s historical trajectory to reconstruct the morphology of our most recent interstellar ...
Hunter Vannier+5 more
doaj +1 more source
Consequences of a Change in the Galactic Environment of the Sun [PDF]
The interaction of the heliosphere with interstellar clouds has attracted interest since the late 1920's, both with a view to explaining apparent quasi-periodic climate "catastrophes" as well as periodic mass extinctions.
Baranov V. B.+17 more
core +2 more sources
The photoreaction induced by Lyman‐α circularly polarized light (CPL) irradiation in racemic alanine film is more complex than simple preferential photolysis of enantiopure alanine molecules, and formation of larger molecules is observed. Circular networks of order of 100 nm scale are introduced in the alanine film surface by the irradiation.
Masahiro Kobayashi+10 more
wiley +1 more source
The QM/MM simulation protocol involving carbonic link bonds was extended for the treatment of layered carbon structures to study the adsorption and intercalation properties of graphitic materials. Abstract The previously introduced workflow to achieve an energetically and structurally optimized description of frontier bonds in quantum mechanical ...
Felix R. S. Purtscher, Thomas S. Hofer
wiley +1 more source
The interface between the outer heliosphere and the inner lism: Morphology of the local interstellar cloud, its hydrogen hole, stromgren shells, and $^{60}$Fe accretion [PDF]
We describe the interface between the outer heliosphere and the local interstellar medium (LISM) surrounding the Sun. The components of the inner LISM are the four partially ionized clouds [the Local Interstellar Cloud (LIC), G cloud, Blue cloud, and Aql cloud] that are in contact with the outer heliosphere, and ionized gas produced by EUV radiation ...
arxiv +1 more source
Microstructure of the Local Interstellar Cloud and the Identification of the Hyades Cloud [PDF]
We analyze high-resolution UV spectra of the Mg II h and k lines for 18 members of the Hyades Cluster to study inhomogeneity along these proximate lines of sight.
Diamond C. J.+14 more
core +2 more sources