4.7 Article

MOLECULAR OUTFLOWS DRIVEN BY LOW-MASS PROTOSTARS. I. CORRECTING FOR UNDERESTIMATES WHEN MEASURING OUTFLOW MASSES AND DYNAMICAL PROPERTIES

Journal

ASTROPHYSICAL JOURNAL
Volume 783, Issue 1, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/783/1/29

Keywords

ISM: clouds; ISM: jets and outflows; stars: formation; stars: low-mass; submillimeter: ISM

Funding

  1. National Aeronautics and Space Administration
  2. National Science Foundation
  3. NASA
  4. Canadian Space Agency
  5. SMA
  6. NSF [AST-0845619]
  7. Deutsche Forschungsgemeinschaft [1573]
  8. Direct For Mathematical & Physical Scien
  9. Division Of Astronomical Sciences [1108907] Funding Source: National Science Foundation
  10. Division Of Astronomical Sciences
  11. Direct For Mathematical & Physical Scien [0845619] Funding Source: National Science Foundation

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We present a survey of 28 molecular outflows driven by low-mass protostars, all of which are sufficiently isolated spatially and/or kinematically to fully separate into individual outflows. Using a combination of new and archival data from several single-dish telescopes, 17 outflows are mapped in (CO)-C-12 (2-1) and 17 are mapped in (CO)-C-12 (3-2), with 6 mapped in both transitions. For each outflow, we calculate and tabulate the mass (M-flow), momentum (P-flow), kinetic energy (E-flow), mechanical luminosity (L-flow), and force (F-flow) assuming optically thin emission in LTE at an excitation temperature, T-ex, of 50 K. We show that all of the calculated properties are underestimated when calculated under these assumptions. Taken together, the effects of opacity, outflow emission at low velocities confused with ambient cloud emission, and emission below the sensitivities of the observations increase outflow masses and dynamical properties by an order of magnitude, on average, and factors of 50-90 in the most extreme cases. Different (and non-uniform) excitation temperatures, inclination effects, and dissociation of molecular gas will all work to further increase outflow properties. Molecular outflows are thus almost certainly more massive and energetic than commonly reported. Additionally, outflow properties are lower, on average, by almost an order of magnitude when calculated from the (CO)-C-12 (3-2) maps compared to the (CO)-C-12 (2-1) maps, even after accounting for different opacities, map sensitivities, and possible excitation temperature variations. It has recently been argued in the literature that the (CO)-C-12 (3-2) line is subthermally excited in outflows, and our results support this finding.

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