Carbon monoxide in the interstellar spectrum of zeta Ophiuchi
Equivalent widths of CO lines in interstellar absorption spectrum of zeta Ophiuchi
Engineering topics
Publications and source records attributed to Stecher, T. P..
Equivalent widths of CO lines in interstellar absorption spectrum of zeta Ophiuchi
Gum Nebula-fossil Stromgren sphere of Vela X supernova, deriving ionization model from interstellar measurements
Interstellar hydrogen ion production and destruction by electron recombination or photodissociation
Galactic gamma rays from OSO-3 observations attributed to decay of neutral pions produced by cosmic rays interaction with interstellar gas nucleons
Galactic gamma ray intensities measured by OSO-3
Stellar spectrophotometry by rocket-borne equipment, describing instrumentation, rocket assembly, calibration and spectra obtained
UV interstellar extinction from comparison of epsilon and zeta Persei, noting graphite features
Planetary nebula formation mechanism based on slow mass loss due to radiation pressure on grains
Positively charged diatomic hydrogen molecules interstellar extinction and photodissociation cross section in terms of formation mechanisms
Interstellar medium polyatomic molecules formation, destruction and excitation processes by astronomical spectroscopy and interferometry
Interstellar extinction in UV from zeta and epsilon Persei spectra obtained with scanner attached to telescope mounted in pointed Aerobee rocket
Spinning rockets UV spectrophotometry of early type stars, discussing instrumentation, calibration, data recording and stellar spectra
Ultraviolet spectra by rocket observations of Zeta Puppis and Gamma Velorum
Localized interstellar molecular hydrogen formation in situations relevant to observations of OB clusters and associations with little H alpha emission
Interstellar SHF radio emission from hydroxyl molecules, discussing maser emission excitation mechanism
Graphite grain formation in stellar atmosphere, analyzing Hoyle-Wickramasinghe condensation mechanism and supersaturation based on nucleation theory
Of and Wolf-Rayet stars high temperature envelopes as cosmic thermal X ray sources, discussing continuous mass loss from spectrophotometry data
Interstellar neutral hydrogen column densities from Lyman alpha measurements noting discrepancies in Orion direction