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Solid co spectroscopy: embedded ysos in taurus-auriga

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Abstract

Infrared spectra of the 4.67µm solid CO feature were obtained for YSOs in Taurus. A first attempt is made to analyse the likely composition of the CO ices. Column densities are derived from the spectra, and compared with the ones predicted for a low mass protostar. The strengths of the CO- and water-ice features towards those objects are compared.

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References

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Authors and Affiliations

  1. Physics Dept., Queen Mary & Westfield College, Mile End Road, E1 4NS, London, UK

    T. C. Teixeira & J. P. Emerson

  2. Centro de Astrofísica da Universidade do Porto, Rua do Campo Alegre 823, 4100, Porto, Portugal

    T. C. Teixeira

Authors
  1. T. C. Teixeira
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  2. J. P. Emerson
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TCT supported by grant BD/2095/92-RM from JNICT- Programa CIENCIA, Portugal

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Teixeira, T.C., Emerson, J.P. Solid co spectroscopy: embedded ysos in taurus-auriga. Astrophys Space Sci 224, 573–574 (1995). https://doi.org/10.1007/BF00667961

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  • DOI: https://doi.org/10.1007/BF00667961

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