Detection of the 12.8-micron Ne super plus emission line from the planetary nebula IC 418.
Detection of micron Ne emission line from planetary nebula IC 418 using IR spectrometer
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Detection of micron Ne emission line from planetary nebula IC 418 using IR spectrometer
Rotational energy conversion of neutron star into relativistic electrons energy suggested by increasing period of pulsating radio source in Crab Nebula
Crab Nebula pulsar properties including pulse shape, dispersion and strong pulse emission
Condensed supernova remnants in Crab Nebula, considering various hypotheses for radio source
IR spectral distribution from region between stars of Trapezium in Orion Nebula
Optical depth at under 110 A due to continuous absorption by N, O and Ne ions estimated in high excitation planetary nebulae
Crab Nebula pulsar detection by TV camera with image intensifier at focus of astronomical telescope, detailing instrumentation and observations
Thermal and free-free emission from planetary nebulae based on graphite grain model, discussing IR fluxes
X ray pulsations in Crab Nebula at frequency closely matching radio and optical pulsations, noting energy distribution
X ray energy spectrum from Crab Nebula and diffuse background on celestial sphere near galactic anticenter, noting spectral index
Pulsar NP 0532 in Crab Nebula observed by rocket and telescope showing strong pulsed X ray signal
Ionization stratification and chemical abundances in planetary nebula NGC 7662, discussing density fluctuations effect on N II and O II lines
Primitive solar nebula physical model considered under angular momentum conservation in collapsing fragment
Ultrarelativistic electron acceleration in Crab Nebula maintaining synchrotron spectrum, obtaining power from compressional motion damping, gyrorelaxation effect and pitch angle anisotropy removal
Rocket measurement of far UV spectral intensity of theta Orionis for far UV interstellar extinction law in Orion nebula region
Photoelectric measurements of emission line intensities for low density planetary nebula with moderate excitation located near north galactic pole, deriving abundances
Tabulation of photographic and photoelectric spectrophotometrically obtained relative spectral line intensities for planetary nebula IC 5217, discussing interstellar absorption
Model for accumulation of earth and planets from primitive solar nebula, implying inhomogeneous chemical composition of bodies in solar system