Stewart Sharpless

Stewart Sharpless

Stewart Sharpless is an American astronomer who carried out fundamental work on the structure of the Milky Way galaxy.

As a graduate student at Yerkes Observatory he worked under William Morgan with fellow graduate student Don Osterbrock.[1] In 1952, they published their observations that demonstrated the spiral structure of the Milky Way by estimating the distances to H II regions and young hot stars. For a while Sharpless was at Mount Wilson Observatory where he worked on galaxy photography with Walter Baade and Edwin Hubble.[2]

In 1953 Sharpless joined the staff of the United States Naval Observatory Flagstaff Station.[2] Here he surveyed and cataloged H II regions of the Milky Way Galaxy using the images from the Palomar Sky Survey. From this work Sharpless published his catalog of H II regions in two editions, the first in 1953 with 142 nebula.[3] The second and final edition was published in 1959 with 313 nebulae[4] (see Sharpless catalog).

Stewart Sharpless is currently a retired Professor Emeritus in the Department of Physics and Astronomy at the University of Rochester.

References

External links

  • Photographic Sharpless Catalog
  • Digitized Sky Survey
  • Stewart Sharpless's home page