Albedo and thermal emission of Jovian satellites I-IV
Albedo and thermal emission of Jovian satellites I-IV at 3 to 12 micron wavelengths
Gillett, F. C.↗
Engineering topics
Stein, W. A.
Publications and source records attributed to Stein, W. A..
The spectrum of VY Canis Majoris from 2.9 to 14 microns
Spectrum of bright IR object VY Canis Majoris, noting absorption feature attributed to SiO molecules in stellar atmosphere
Gillett, F. C.↗
Cosmic sources of infrared radiation
Cosmic IR radiation sources, discussing galactic and stellar masses
Burbidge, G. R.↗
Spectra of ''infrared stars'' from 2.8 to 5.1 microns
Low resolution spectra of IR stars NML Tau, CIT 3, 6 and 13 considered inadequate for molecular band identification
Gaustad, J. E.↗
The 2.8-14-micron spectrum of Jupiter.
Jupiter spectrum observations in 2.8-14 micron range, describing absorption strength and brightness temperature, basing analysis on ammonia, methane and hydrogen absorption
Gillett, F. C.↗
The spectrum of NML Cygnus from 7.5 to 14 microns.
Spectrum of IR object NML Cygnus, discussing model based on circumstellar IR emission
Gaustad, J. E.↗
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.↗
Spectral distribution of infrared radiation from the Trapezium region of the Orion Nebula.
IR spectral distribution from region between stars of Trapezium in Orion Nebula
Gillett, F. C.↗
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
Gillett, F. C.↗
Circumstellar infrared emission from two peculiar objects - R Aquarii and R Coronae Borealis.
IR excess from carbon-rich peculiar variable R Coronae Borealis and M7 variable associated with emission nebula R Aquarii attributed to circumstellar matter
Gaustad, J. E.↗
X-rays from the Coma cluster of galaxies
X ray source from Coma cluster of galaxies, interpreting observed flux on basis of missing mass suggested by Virial theorem
Felten, J. E.↗
Stellar spectra from 2.8 to 14 microns.
Stellar spectra observed with 2.8-14 micron IR spectrometer, noting broad absorption feature near 5 and 8 microns
Gillett, F. C.↗
The spectrum of NML Cygnus from 2.8 to 5.6 microns.
IR spectrum of NML Cygnus, discussing weak absorption band
Gillett, F. C.↗
Absolute spectrum of Venus from 2.8 to 14 microns.
Venus absolute spectrum in 2.8-14 micron range, noting strong sunlight absorption in 3-5 micron region and low brightness temperature between 8-10 microns
Gillett, F. C.↗
Observations of the Crab Nebula at lambda equals 5800 angstron units nu, and 3.5 nu with a 4-minute beam.
IR observations of Crab Nebula using 30 inch aperture telescope
Ney, E. P.↗
Infrared observations of the planetary nebula NGC 7027.
IR line intensity of planetary nebula NGC 7027, noting presence of measurable continuum flux of stellar radiation
SPECTRAL LINE↗
Infrared continuum from H II regions.
Detectability of ion recombination free-free emission from H II regions
CONTINUUM RADIATION↗