Summary
Bengt Westerlund (January 17, 1921 - June 4, 2008)[1][2] was a Swedish astronomer who specialised in observational astronomy.
He received his PhD from Uppsala University in 1954.[2] In 1957 he was appointed astronomer at the Uppsala Southern Station at Mount Stromlo Observatory in Australia, where he made extensive studies of the southern Milky Way and the Magellanic Clouds.[1] In 1967 he took a position as astronomer at Steward Observatory in Arizona and in 1969 was appointed Director of ESO in Chile, a position he held until 1975, when he returned to Sweden to become Professor of Astronomy at Uppsala Astronomical Observatory, retiring in 1987.[2]
Work edit
His work on the structure of the Milky Way and the Magellanic Clouds was held in high regard. He contributed significantly in studies of star clusters, stellar populations, carbon stars, planetary nebulae, Wolf-Rayet stars, stellar classification and supernova remnants.[2] He was regarded as an expert on the Magellanic Clouds[1] and wrote a book on them (The Magellanic Clouds, Cambridge University Press, 1997 ISBN 0521480701).
Discoveries edit
He discovered or rediscovered three open star clusters, Westerlund 1, Westerlund 2 and Westerlund 3.[3] He also discovered the red supergiant, WOH G64.[4]
Honors edit
Namesakes edit
Asteroid 2902 Westerlund was named after him when he retired from his professorship and the Westerlund telescope in Uppsala was named in his honour in 2004.[1]
References edit
- ^ a b c d "Bengt Westerlund (1921-2008)". Uppsala University. Archived from the original on 28 December 2014. Retrieved 9 May 2015.
- ^ a b c d "In Memoriam: Bengt Westerlund" (PDF). ESO.org. Archived from the original (PDF) on 24 September 2015. Retrieved 9 May 2015.
- ^ Archinal, Brent; Hynes, Steven (2003). Star Clusters. Willmann-Bell. p. 195. ISBN 0943396808.
- ^ Westerlund, B. E.; Olander, N.; Hedin, B. (1981). "Supergiant and giant M type stars in the Large Magellanic Cloud". Astronomy & Astrophysics Supplement Series. 43: 267–295. Bibcode:1981A&AS...43..267W.