Results 101 to 110 of about 110,978 (225)
On the Abiotic Origin of Dimethyl Sulfide: Discovery of Dimethyl Sulfide in the Interstellar Medium
Following the discovery of dimethyl sulfide (DMS; CH _3 SCH _3 ) signatures in comet 67P/Churyumov–Gerasimenko, we report the first detection of this organosulfur species in the interstellar medium during the exploration of an ultradeep molecular line ...
Miguel Sanz-Novo+16 more
doaj +1 more source
Shock waves in Interstellar Cloud-Cloud and Wind-Cloud Collisions [PDF]
The interstellar medium (ISM) is a key ingredient of galaxies and their evolution, consisting of multiphase, turbulent dust and gas. Some of the star-forming regions in our Galaxy originate from cloud-cloud and wind-cloud collisions, which generate shock waves that change the physical and chemical properties of the gas.
arxiv +1 more source
A primary goal of the FUSE mission is to understand the origin of the O VI ion in the interstellar medium of the Galaxy and the Magellanic Clouds. Along sightlines to OB-type stars, these interstellar components are usually blended with O VI stellar wind
A. W. Fullerton+6 more
core +1 more source
Accurate interpretation of observations relies on the interstellar dust extinction law, which also serves as a powerful diagnostic for probing dust properties.
Juan Deng+3 more
doaj +1 more source
Interstellar extinction is investigated in a 1.5 square degree area of the Cepheus Flare in the direction of the dark cloud TGU 619 at ℓ=102.5°, b=+15.5°.
Zdanavičius K.+4 more
doaj +1 more source
The Expansion of an Interstellar Gas-Cloud into a Vaccum* [PDF]
G. C. McVittie
openalex +1 more source
The Spectral Energy Distribution of Self-gravitating Interstellar Clouds I. Spheres
We derive the spectral energy distribution (SED) of dusty, isothermal, self gravitating, stable and spherical clouds externally heated by the ambient interstellar radiation field.
Bernard J. P.+17 more
core +1 more source
10. Radio observations of interstellar neutral hydrogen clouds [PDF]
Robert S. Lawrence
openalex +1 more source
Random independent splitting model for the mass spectrum of protostars and interstellar clouds [PDF]
Mathematical model for mass spectra of protostars and interstellar ...
Marcus, A. H.
core +1 more source
Is the Sun Embedded in a Typical Interstellar Cloud?
The physical properties and kinematics of the partially ionized interstellar material near the Sun are typical of warm diffuse clouds in the solar vicinity.
A. Czechowski+57 more
core +1 more source