Henrietta Hill Swope's AcademicInfluence.com Rankings Henrietta Hill Swope's Degrees Why Is Henrietta Hill Swope Influential? (Suggest an Edit or Addition)
According to Wikipedia , Henrietta Hill Swope was an American astronomer who studied variable stars. In particular, she measured the period-luminosity relation for Cepheid stars, which are bright variable stars whose periods of variability relate directly to their intrinsic luminosities. Their measured periods can therefore be related to their distances and used to measure the size of the Milky Way and distances to other galaxies.
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1950 1960 1970 0 5 10 15 20 25 30 35 40 45 50 55 60 65 70 Published Works Variable star field 96' south preceeding the nucleous of the Andromeda galaxy. (1963) The Draco system, a dwarf galaxy. (1961) Variables in the Andromeda galaxy - Fields I and III. (1965) Progress Report on the Leo II System (1967) 37. Star Clusters and Associations (1970) The Palomar survey of variables in M 31 (First results). (1955) Note on planetary nebulae in M31 (1963) Variations of CL and HK Scorpii. (1941) A study of the magnitudes and colors of the globular cluster NGC 6397. (1952) LORAN: The Planning, Growth, and Use of Loran, the New Long‐Range Aid to Navigation* (1946) V2283 Sgr, an eclipsing star with a rotating apse. (1974) (1)Two Hundred and Twenty-four New Variable Stars in Scorpio and Ophiuchus (1928) (0)MEETING OF THE EIGHTH GENERAL ASSEMBLY OF THE INTERNATIONAL ASTRONOMICAL UNION (1953) UX Lupi. a Sixteen-day Cepheid (1941) (0)Milky Way Field Measures (0)Long Period Variables in MWF 176 (1930) (0)Eclipsing Binaries with Apsidal Motion (1938) (0)Charts for Faint Variable Stars, Second Series: Milky Way Field 185 (1932) (0)Variable measures MWF 187c (1942) (0)Variable stars in the southern third of MWF 187 (1942) (0)Variable stars in MWF 189 (1940) (0)Variables, MWF 179, MWF 187 (0)A peculiar variable with changing period and light curve (1937) (0)The Variable Stars of Milky Way Field 239 (1941) (0)Studies of the Galactic Center: II. Preliminary Indication of a Massive Galactic Nucleus. (1928) A FAINT NOVA IN OPHIUCHUS (JULY 1940) (1941) Periods of Thirty~five Cluster Type Cepheids in Milky Way Field 185 (0)Prediscovrery Photographic Observations of SS Cygni (1941) (0)MIlky Way Field 185 Positions, Magnitude Estimates, Sequences (0)More Papers This paper list is powered by the following services:
Other Resources About Henrietta Hill Swope What Schools Are Affiliated With Henrietta Hill Swope? Henrietta Hill Swope is affiliated with the following schools:
