Interplanetary gas. XVII - An astrometric determination of solar-wind velocities from orientations of ionic comet tails.
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Engineering topics
Publications and source records attributed to Roosen, R. G..
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Results of photoelectric observations in B and V made at over 1200 locations in Messier 81, covering an area of approximately 169 square minutes of arc and including the galaxy's nucleus. Isophote maps in V and B based on these observations have been drawn. Two independent fits on the resulting V and B luminosity distributions yield average integrated magnitudes of V equals 6.94 and B equals 7.89. B - V and (integrated B) - (integrated V) are given as functions of distance from the center of the galaxy along the semimajor axis. A mass model is derived using a rotation curve based on the velocities measured by Muench (1959). The total mass of M81 is found to be 1.62 x 10 to the 11th solar masses. The final apparent mass-to-luminosity ratios in V and B are 11.2 and 15.1, respectively.
Several years of observational results are available from the Pioneer 8 and 9 interplanetary dust detectors, and these data were used to show dust counts graphically. The characteristics of the five largest dust showers are also summarized.
Gegenschein observational history and characteristic features, discussing theories regarding origin
Hypothetical geocentric /interplanetary/ dust cloud concentration detection possibility by earth shadow
Zodiacal light brightness measurement in three mutually perpendicular directions, tabulating data
Bibliography on Gegenschein covering observations, theories, models, review papers, etc
Gegenschein photographic and photoelectric scan observations, considering origin in light reflection from interplanetary dust outside earth orbit
Libration clouds reality possibility from satellite dust counting experiments
Radio galaxy Messier 87 mass determined using virial theorem for nucleus velocity dispersion