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Category: Classical

Doradus Stars

by Tygohn

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  1. Jun 28,  · The star-forming region, 30 Doradus, is one of the largest located close to the Milky Way and is found in the neighboring galaxy Large Magellanic Cloud. About 2, massive stars in the center of 30 Doradus, also known as the Tarantula Nebula, are producing intense radiation and powerful winds as they blow off material.
  2. The star-forming region, 30 Doradus, is one of the largest located close to the Milky Way and is found in the neighboring galaxy, Large Magellanic Cloud. About 2, massive stars in the center of 30 Doradus, also known as the Tarantula Nebula, are producing intense radiation and powerful winds as they blow off material.
  3. Dorado is composed mainly of dim stars. The brightest star is Alpha Doradus with a visual magnitude of It is a binary star system located approximately light years from Earth. The second brightest star is Beta Doradus.
  4. Seven of these new γ Doradus stars appear to be single, three are primaries of single-lined binaries, and one has two distant visual companions; none are double-lined or close visual binaries. Several of the stars show spectroscopic line-profile and low-amplitude radial velocity variability indicative of pulsation.
  5. XY Doradus is a m1iii giant star that can be located in the constellation of Dorado. The description is based on the spectral class. XY Doradus is not part of the constellation outline but is within the borders of the constellation. Based on the spectral type (M1III) of the star, the star's colour is red.
  6. S Doradus is a supergiant star that can be located in the constellation of Dorado. The description is based on the spectral class. S Doradus is not part of the constellation outline but is within the borders of the constellation. Based on the spectral type (B8/9eq – .
  7. Spectroscopy of γ Doradus stars - Volume 9 Issue S - E. Brunsden, K. R. Pollard, P. L. Cottrell, D. J. Wright, P. De Cat, P. M. Kilmartin.
  8. Oct 01,  · The Gamma Doradus variables are a newly discovered class of multiperiodic variable stars, found mainly among main-sequence stars at or near the cool border of Delta Scuti star instability strip. Evidence for this new class of pulsating stars was presented by Balona, Krisciunas & Cousins (), who photometrically examined the star Gamma Doradus Author: M. Breger, G. Handler, R. Garrido, N. Audard, F. Beichbuchner, W. Zima, M. Paparo, Z. Li, S. Jiang.

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