Last edited by Vijar
Saturday, May 9, 2020 | History

2 edition of Twenty-four southern perculiar emissionline stars. found in the catalog.

Twenty-four southern perculiar emissionline stars.

Eric Dungan Carlson

Twenty-four southern perculiar emissionline stars.

by Eric Dungan Carlson

  • 239 Want to read
  • 22 Currently reading

Published in Evanston, Ill .
Written in English

    Subjects:
  • Stars -- Observations,
  • Stars -- Spectra,
  • Milky Way

  • Edition Notes

    GenreObservations
    Classifications
    LC ClassificationsQB818 C35 1968A
    The Physical Object
    Pagination[225 leaves]
    Number of Pages225
    ID Numbers
    Open LibraryOL19747067M

    They are implemented for training Gaia data analysis algorithms for the classification of a wide variety of hot and cool star types; FGK and M stars, OB stars, white dwarfs, red supergiants, peculiar A and B stars, carbon stars, ultra cool dwarfs, various types of emission line stars, Be stars, Wolf–Rayet stars Author: Walter Van Rensbergen. WR 31a, commonly referred to as Hen , is a Wolf–Rayet (WR) star in the southern constellation of Carina that is surrounded by an expanding Wolf–Rayet is not a classical old stripped-envelope WR star, but a young massive star which still has some hydrogen left in its llation: Carina.

    10 Southern books we want to read in Things to do. The first third of the new year promises a slew of thrilling new books that are penned by Southern-based authors or take place in the Author: Suzanne Van Atten. In addition to teaching, he conducted research on planetary nebulae, peculiar emission-line stars, S-stars, and T-associations. During and , he was a guest observer at Mt. Stromlo Observatory in Canberra, Australia, where he used instruments ranging from the Uppsala 20/inch schmidt to the inch parabolic reflector.

    An astronomical catalogue is a list or tabulation of astronomical objects, typically grouped together because they share a common type, morphology, origin, means of detection, or method of omical catalogs are usually the result of an astronomical survey of some kind. Others contain one or two stars of the first or second magnitude, and then a greater or less variety of lesser stars; but this is peculiar from having no one very bright star, but contains so many stars of the 4th and 5th magnitudes. It contains 43 stars altogether, ten being of the 4th magnitude, and the remainder of the 5th, 6th, etc.


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Twenty-four southern perculiar emissionline stars by Eric Dungan Carlson Download PDF EPUB FB2

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TWENTY SOUTHERN PECULIAR EMISSION-LINE STARS Eric D. Carlson* and Karl G. Henize** 'The Adler Planetarium, Chicago, Illinois **NASA Lyndon B. Johnson Space Center, Houston, Texas I INTRODUCTION Observational data are presented for 20 peculiar emission-line stars located in the southern Cited by: adshelp[at] The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86AAuthor: E.

Carlson. Observational data for 20 southern stars having emission-line spectra that suggest a significant degree of mass ejection are given in order to present an atlas of Twenty-four southern perculiar emissionline stars.

book spectra and to give a quantitative description of their appearance during the epoch. Most of the stars are P Cygni stars; others include nova-like, peculiar Be, and symbiotic stars, as well as stellar planetary nebulae. Southern Stars book. Read 15 reviews from the world's largest community for readers.

At last, Dar and Kerry get to go on their long awaited and anticipat /5. Twenty southern peculiar emission-line stars. southern stars having emission-line spectra that suggest a significant degree of mass ejection are given in order to present an atlas of their spectra and to give a quantitative description of their appearance during the epoch.

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HD may be considered the prototype for these peculiar emission-line stars that are now called B[e]'s, i.e. Be stars whose spectra exhibit forbidden lines as well as permitted lines of H, Fe II, HD has the following coordinates: alpha = 6/m and delta ='.

Most of the stars are P Cygni stars; others include nova-like, peculiar Be, and symbiotic stars, as well as stellar planetary nebulae and emission-line binaries, all of whose spectra were obtained. Explore releases from Southern All Stars at Discogs. Shop for Vinyl, CDs and more from Southern All Stars at the Discogs Marketplace.

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In addition to teaching, he conducted research on planetary nebulae, peculiar emission-line stars, S-type stars, and T-associations. During andhe was a guest observer at Mount Stromlo Observatory in Canberra, Australia, where he used instruments ranging from the Uppsala 20/inch schmidt to the inch parabolic reflector.