Tom Bolton
Born
Charles Thomas Bolton

(1943-04-15)April 15, 1943
Tullahoma, Tennessee, U.S.
Diedc. February 4, 2021 (aged 77)
Richmond Hill, Ontario, Canada
Alma materUniversity of Illinois
University of Michigan
Known forEvidence for Stellar-mass black holes
AwardsFellow of the Royal Society of Canada
Scientific career
FieldsAstronomy
InstitutionsDavid Dunlap Observatory, University of Toronto

Charles Thomas Bolton (April 15, 1943 – c. February 4, 2021)[1] was an American-Canadian astronomer who was one of the first in his field to present strong evidence of the existence of a stellar-mass black hole.[2][3]

Biography

Bolton was born in Camp Forrest, a military base in Tullahoma, Tennessee.[2] He received his bachelor's degree in 1966 from the University of Illinois, followed by a 1968 master's degree and a 1970 doctoral degrees from the University of Michigan.[2]

Bolton then worked as a postdoctoral researcher at the David Dunlap Observatory in Richmond Hill, Ontario, teaching there until 1972.[2] He taught at Scarborough College from 1971 to 1972, and at Erindale College from 1972 to 1973. Thereafter, he was affiliated with the University of Toronto astronomy department,[2] eventually becoming an emeritus professor.[4]

In 1970, Bolton developed the first computer models for stellar spectra that were precise enough to compare with data from real stars.[2]

In 1971, as a post-doctoral fellow and part-time faculty member studying binary systems at the Dunlap Observatory,[5][6] Bolton observed star HDE 226868 wobble as if it were orbiting around an invisible but massive companion emitting powerful X-rays,[2][7] independently of the work by Louise Webster and Paul Murdin, at the Royal Greenwich Observatory.[8] Further analysis gave an estimate about the amount of mass needed for the gravitational pull, which proved to be too much for a neutron star. After more observations confirmed the results, by 1973, the astronomical community generally recognized black hole Cygnus X-1, lying in the plane of the Milky Way galaxy at a galactic latitude of about 3 degrees.[2][9][10][11]

In 1985, Bolton and Douglas Gies showed that hot, massive "runaway OB stars" (stars that travel at an abnormally high velocity relative to the surrounding interstellar medium), could be accelerated through stellar interactions within star clusters, in addition to being ejected from binary systems after supernova explosions.[12][2]

Bolton was instrumental in passing the first light-pollution regulation Canada, a 1995 bylaw to limit light pollution in the town Richmond Hill, home of the David Dunlap Observatory.[2][13] He was a fellow of the Royal Society of Canada.[2] Bolton died in February 2021, at his home in Richmond Hill.[14]

References

  1. ↑ "Astronomer Tom Bolton found compelling evidence of a black hole's existence". The Globe and Mail. 2021-02-19. Retrieved 2022-01-31.
  2. 1 2 3 4 5 6 7 8 9 10 11 "Charles Thomas Bolton (1943- )". Virtual Museum of Canada. Retrieved 2007-07-05.
  3. ↑ Black, Harry (2008). "Tom Bolton, Astronomer: Discoverer of the First Black Hole". Canadian Scientists and Inventors: Biographies of People Who Shaped Our World. Pembroke Publishers Limited. pp. 24–27. ISBN 978-1-55138-222-7..
  4. ↑ Faculty profile Archived 2012-07-18 at archive.today, U. of Toronto Astronomy and Astrophysics Dept.
  5. ↑ Culp, Kritine. "The proof is out there". University of Toronto Magazine. Retrieved 2008-07-06.
  6. ↑ "Black holes: The Canadian connection". Quirks and Quarks. CBC. 2008-04-18. Retrieved 2008-07-05.
  7. ↑ Bolton, C. T. (1972). "Identification of Cygnus X-1 with HDE 226868". Nature. 235 (5336): 271–273. Bibcode:1972Natur.235..271B. doi:10.1038/235271b0. S2CID 4222070.
  8. ↑ Webster, B. Louise; Murdin, Paul (1972). "Cygnus X-1—a Spectroscopic Binary with a Heavy Companion?". Nature. 235 (5332): 37–38. Bibcode:1972Natur.235...37W. doi:10.1038/235037a0. S2CID 4195462.
  9. ↑ Rolston, Bruce (November 10, 1997). "The First Black Hole". University of Toronto. Archived from the original on 2008-03-07. Retrieved 2008-03-11.
  10. ↑ Shipman, H. L. (1975). "The implausible history of triple star models for Cygnus X-1 Evidence for a black hole". Astrophysical Letters. 16 (1): 9–12. Bibcode:1975ApL....16....9S. doi:10.1016/S0304-8853(99)00384-4.
  11. ↑ Gursky, H.; Gorenstein, P.; Kerr, F. J.; Grayzeck, E. J. (1971). "The Estimated Distance to Cygnus X-1 Based on its Low-Energy X-Ray Spectrum". Astrophysical Journal. 167: L15. Bibcode:1971ApJ...167L..15G. doi:10.1086/180751.
  12. ↑ Gies, D. R.; Bolton, C. T. (1986). "The binary frequency and origin of the OB runaway stars". The Astrophysical Journal Supplement Series. 61: 419. Bibcode:1986ApJS...61..419G. doi:10.1086/191118. ISSN 0067-0049.
  13. ↑ "Lights out for pollution | The Star". thestar.com. Retrieved 2018-10-30.
  14. ↑ Alexander W. Fullerton, Douglas R. Gies, Ian K. Shelton, and Steven N. Shore (April 13, 2021). "Charles Thomas Bolton (1943–2021)". Bulletin of the American Astronomical Society. Vol. 53, no. 2. Retrieved January 9, 2022.{{cite magazine}}: CS1 maint: multiple names: authors list (link)
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.