Wavelength dependence of polarization. 9 - Interstellar particles
Wavelength dependence of interstellar polarization
Gehrels, T.↗
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Carbon 12 to carbon 13 ratio in the interstellar medium
Carbon 12 to carbon 13 ratio in Zeta Ophivchi and exchange with interstellar matter
Thaddeus, P.↗
The dynamical state of the interstellar gas and field. VI - Instability and enhanced diffusion in a twisted field.
Interstellar gas field dynamic instability, discussing enhanced ambipolar diffusion in twisted field
Lerche, I.↗
Detection of NH sub 3 molecules in the interstellar medium by their microwave emission.
Ammonia gas molecules in interstellar medium, discussing detection in direction of galactic center by means of microwave emission
Cheung, A. C.↗
Detection of water in interstellar regions by its microwave radiation.
Water in interstellar regions detected by microwave emission from 6 sub 16 to 5 sub 23 rotational transition
Cheung, A. C.↗
The dynamical state of the interstellar gas and fields. VII.
Attractive and disruptive forces in conversion of interstellar gas into stars, discussing self gravitation, galactic magnetic field and cosmic ray pressure
Parker, E. N.↗
Interstellar polarization and galactic magnetic field strengths.
Polarization to extinction ratio criterion to choose interstellar cloud model, discussing magnetic field strength requirements
Greenberg, J. M.↗
Extinction by interstellar grains, Mie particles and polycyclic aromatic molecules.
Interstellar extinction models of classical Mie particles and quantum mechanical polycyclic aromatic molecules
Donn, B.↗
A possible identification of interstellar silicate absorption in the infrared spectrum of 119 Tauri.
Reddened M supergiant 119 Tauri IR spectra and IR absorption by CO and SiO molecules in stellar atmosphere and silicate mineral in interstellar grains
Gaustad, J. E.↗
Microwave detection of interstellar formaldehyde.
Interstellar formaldehyde detection in absorption against galactic and extragalactic radio sources, discussing chemical evolution
Buhl, D.↗
Solid hydrogen coated graphite particles in the interstellar medium. I.
Solid para hydrogen coated graphite particles expulsion into interstellar medium from star formation regions, considering mantles stability and particles extinction efficiency, albedo and phase function
Swamy, K. S. K.↗
Interstellar absorption of 10-angstrom X-rays.
Interstellar absorption of 10 A X rays from sources in Scorpio-Sagittarius region, noting gas density between earth and Crab Nebula
Bradt, H. V.↗
Local interstellar reddening.
Interstellar reddening in solar vicinity, analyzing roles of galactic latitude and longitude and heliocentric distance
Gottlieb, D. M.↗
On the far-ultraviolet interstellar extinction law in the Orion nebula region.
Rocket measurement of far UV spectral intensity of theta Orionis for far UV interstellar extinction law in Orion nebula region
Carruthers, G. R.↗
Interstellar polarization of starlight and the turbulent structure of the Galaxy.
Polarization fluctuations of starlight indicating turbulent structure of interstellar medium, noting pulsar signal dispersion and Faraday rotation
Jokipii, J. R.↗
Interstellar extinction in the ultraviolet. II.
Interstellar extinction in UV from zeta and epsilon Persei spectra obtained with scanner attached to telescope mounted in pointed Aerobee rocket
Stecher, T. P.↗
Detection of interstellar H sub 2 C super 13 O super 16.
Carbon isotopes compared in interstellar formaldehyde transition for galactic nucleosynthesis, discussing spectrum analysis of radio astronomical telescope observations
Buhl, D.↗
The interstellar H super plus sub 2 molecule.
Positively charged diatomic hydrogen molecules interstellar extinction and photodissociation cross section in terms of formation mechanisms
Stecher, T. P.↗