Discovery of a Low-Mass Bipolar Molecular Outflow from L1014-IRS with the Submillimeter Array

  • Bourke T
  • Crapsi A
  • Myers P
  • et al.
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Abstract

Using the Submillimeter Array we report the discovery of a compact low mass bipolar molecular outflow from L1014-IRS and confirm its association with the L1014 dense core at 200 pc. Consequently, L1014-IRS is the lowest luminosity (L \~0.09 Lsun) and perhaps the lowest mass source known to be driving a bipolar molecular outflow, which is one of the smallest known in size (~500 AU), mass (< 10^{-4} Msun), and energetics (e.g., force < 10^{-7} Msun km/s/yr).

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Bourke, T. L., Crapsi, A., Myers, P. C., Evans II, N. J., Wilner, D. J., Huard, T. L., … Young, C. H. (2005). Discovery of a Low-Mass Bipolar Molecular Outflow from L1014-IRS with the Submillimeter Array. The Astrophysical Journal, 633(2), L129–L132. https://doi.org/10.1086/498449

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