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Robert Michael Rich (born 1957) is an American astrophysicist. He obtained his B.A. at Pomona College in 1979 and earned his Ph.D. from the California Institute of Technology in 1986 under thesis supervisor Jeremy R. Mould.
About R. Michael Rich. I work on the subject of "Galactic archeology" - the ages, chemistry, kinematics, and structure of stellar populations at the present epoch (the "fossil record") as a constraint and primary source of information on theories of galaxy formation and evolution.
R. Michael Rich. My principle research interest is in the Galactic bulge and stellar populations. I am interested in the age and origin of the bulge and thick disk, and the relationship of those populations to the inner halo and globular clusters.
R. Michael Rich mainly investigates Astrophysics, Astronomy, Galaxy, Stars and Globular cluster. His Astrophysics research focuses on Bulge, Metallicity, Star formation, Milky Way and Radial velocity.
R. Michael Rich's 821 research works with 40,710 citations and 2,920 reads, including: COSMOS-Web: Intrinsically Luminous z$\gtrsim$10 Galaxy Candidates Test Early Stellar Mass Assembly.
Tracing the rise of supermassive black holes: A panchromatic search for faint, unobscured quasars at z > 6 with COSMOS-Web and other surveys. Introducing the Condor Array Telescope – III. The expansion and age of the shell of the dwarf nova Z Camelopardalis, and detection of a second, larger shell.
Robert Michael Rich, American Astronomy educator. Achievements include co-discovery of metal-rich stars in the galacticbulge; establishment of wide metal abundance range in bulge and linkto galaxy populations; first extragalactic detection of diffuse interstellar bands, luminosity function and properties of stars in the bulge of M31 ...
