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Showing papers in "The Astrophysical Journal in 1969"


Journal Article•DOI•

987 citations


Journal Article•DOI•

806 citations




Journal Article•DOI•
TL;DR: Two armed spiral galactic shock waves as triggering mechanism for gravitational collapse leading to star formation, considering gaseous disk motion using Schmidt model, were proposed in this article, where the authors used the Schmidt model for star formation.
Abstract: Two armed spiral galactic shock waves as triggering mechanism for gravitational collapse leading to star formation, considering gaseous disk motion using Schmidt model

610 citations


Journal Article•DOI•
TL;DR: Pulsar model with seat as rotating neutron star having dipolar magnetic field not parallel to rotation axis is presented in this article, where the magnetic field is not parallel with the rotation axis.
Abstract: Pulsar model with seat as rotating neutron star having dipolar magnetic field not parallel to rotation axis

526 citations



Journal Article•DOI•

492 citations


Journal Article•DOI•
TL;DR: Optically thin gas surrounding X ray source, plotting electron temperature and ionization equilibrium of hydrogen, He, carbon, nitrogen, oxygen and neon as mentioned in this paper, was used to calculate the equilibrium of electron temperature.
Abstract: Optically thin gas surrounding X ray source, plotting electron temperature and ionization equilibrium of hydrogen, He, carbon, nitrogen, oxygen and neon

440 citations


Journal Article•DOI•
TL;DR: Density wave theory of galactic spirals, discussing hydrogen distribution, young star distribution, stellar migration, magnetic field structure, density waves in stellar formation, etc as discussed by the authors, etc.
Abstract: Density wave theory of galactic spirals, discussing hydrogen distribution, young star distribution, stellar migration, magnetic field structure, density waves in stellar formation, etc

431 citations



Journal Article•DOI•
TL;DR: Ionization equilibrium and radiative cooling of high temperature low density plasma, noting cosmic gas cooling curve of line emission from oxygen ion transitions, were discussed in this paper, where the authors also showed that the line emission of oxygen ion transition can be seen as a sign of low-density plasma.
Abstract: Ionization equilibrium and radiative cooling of high temperature low density plasma, noting cosmic gas cooling curve of line emission from oxygen ion transitions

Journal Article•DOI•
TL;DR: Stochastic and ergodic aspects of magnetic lines of force, discussing cosmic ray diffusion in interplanetary magnetic field are discussed in this article, where the authors also consider the effects of cosmic ray on the magnetic field.
Abstract: Stochastic and ergodic aspects of magnetic lines of force, discussing cosmic ray diffusion in interplanetary magnetic field


Journal Article•DOI•
TL;DR: In this article, solar wind-induced torque calculated considering special and general relativistic effects, extending method to pulsar rotational model was presented. But the method was not suitable for the pulsar model.
Abstract: Solar wind-induced torque calculated considering special and general relativistic effects, extending method to pulsar rotational model

Journal Article•DOI•
TL;DR: In this article, the intensity, spectrum and polarization of gyrosynchrotron radiation from magnetoactive plasma electrons distribution are analyzed. But the authors focus on magneto-active plasma electron distribution.
Abstract: Intensity, spectrum and polarization of gyrosynchrotron radiation from magnetoactive plasma electrons distribution


Journal Article•DOI•
TL;DR: Group velocity of spiral density waves propagating in disk galaxies implying self-destruction, discussing possible replenishment sources as mentioned in this paper. But the authors did not consider the effects of the density wave on the galaxies.
Abstract: Group velocity of spiral density waves propagating in disk galaxies implying self destruction, discussing possible replenishment sources


Journal Article•DOI•
TL;DR: In this article, the mass and radius relations for zero temperature spheres of chemical elements, using equation of state and numerical integration, were derived for zero-temperature spheres of the chemical elements.
Abstract: Mass and radius relations for zero temperature spheres of chemical elements, using equation of state and numerical integration


Journal Article•DOI•
TL;DR: Infinitesimal bending oscillations and/or responses of thin rotating disks applied to thin disk galaxies are discussed in this article, discussing Magellanic Cloud passage near galactic center.
Abstract: Infinitesimal bending oscillations and/or responses of thin rotating disks applied to thin disk galaxies, discussing Magellanic Cloud passage near galactic center

Journal Article•DOI•
TL;DR: Doubling principle providing rapid and accurate results for problem of diffuse reflection from plane parallel atmosphere as mentioned in this paper, where the doubling principle was used to solve the problem of diffusing reflection from parallel atmosphere.
Abstract: Doubling principle providing rapid and accurate results for problem of diffuse reflection from plane parallel atmosphere



Journal Article•DOI•
TL;DR: Bolometric luminosity-red shift relations of Friedmann dust universes corrected for inhomogeneities, using locally inhomogeneous Swiss cheese models as discussed by the authors, were used to calculate the luminosity and red shift relations.
Abstract: Bolometric luminosity-red shift relations of Friedmann dust universes corrected for inhomogeneities, using locally inhomogeneous Swiss cheese models


Journal Article•DOI•
TL;DR: Broadband photometry for circumstellar IR emission from cool stars, considering giant and carbon stars, was proposed in this paper, where the authors considered two types of stars, namely, the giant and the carbon stars.
Abstract: Broadband photometry for circumstellar IR emission from cool stars, considering giant and carbon stars

Journal Article•DOI•
TL;DR: In this paper, the authors calculate molecular equilibrium of condensates and gaseous compounds in stellar atmospheres using O to C abundance ratios of stars with various O-to-C abundance ratios.
Abstract: Circumstellar grain compositions of stars with various O to C abundance ratios, calculating molecular equilibrium of condensates and gaseous compounds in stellar atmospheres