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The Possible Determination of Two New BL Lac Redshifts

  • M. Persic
  • P. Salucci
Part of the Astrophysics and Space Science Library book series (ASSL, volume 121)

Abstract

We present tentative identifications of very faint emission lines in the spectra of the BL Lacertae objects 0754+100 and 1514+197 as given in the atlas of spectra of QSOs and related objects by Wilkes et. al.(1983). The proposed identifications, quite common in BL Lac spectra, are discussed.

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References

  1. Danziger,I.J., Fosbury,R.A.E., Goss,W.M.: 1978, in Pittsburgh Conference on BL Lac Objects, Ed. A.M. Wolfe, Univ. of Pittsburgh, Pittsburgh, pennsylvania, 204.Google Scholar
  2. Meinel,A.B., Aveni,A.F., Stockton,M.W.: 1968, Catalog of Emission Lines in Astrophysical Objects, The University of Arizona, Tucson.Google Scholar
  3. Miller,J.S., French,H.B.: 1978, in Pittsburgh Conforence on BL Lac Objects, Ed. A.M. Wolfe, Univ. of Pittsburgh, Pittsburgh, Pennsylvania, 228.Google Scholar
  4. Miller,J.S., French,H.B., Hawley,S.A.: 1978, in Pittsburgh Conference on BL Lac Objects, Ed. A.M. Wolfe, Univ. of Pittsburgh, Pittsburgh, Pennylvania, 176.Google Scholar
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  6. Urry, C.M.: 1984, NASA Technical Memorandum 86103.Google Scholar
  7. Wilkes,B.J., Wright,A.E., Jauncey,D.L., Peterson,B.A.: 1983, Proc. Astron. Soc. Australia, Vol.5, No.1, 2.ADSGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1986

Authors and Affiliations

  • M. Persic
    • 1
    • 2
  • P. Salucci
    • 1
    • 2
  1. 1.SISSA-ISASMiramare, TriesteItaly
  2. 2.Osservatorio AstronomicoTriesteItaly

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