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arXiv · 1401.0455

SMA Submillimeter Observations of HL Tau: Revealing a compact molecular outflow

Alba M. Lumbreras·Luis A. Zapata
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Abstract

We present archival high angular resolution ($\sim$ 2$''$) $^{12}$CO(3-2) line and continuum submillimeter observations of the young stellar object HL Tau made with the Submillimeter Array (SMA). The $^{12}$CO(3-2) line observations reveal the presence of a compact and wide opening angle bipolar outflow with a northeast and southwest orientation (P.A. = 50$^\circ$), and that is associated with the optical and infrared jet emanating from HL Tau with a similar orientation. On the other hand, the 850 $\mu$m continuum emission observations exhibit a strong and compact source in the position of HL Tau that has a spatial size of $\sim$ 200 $\times$ 70 AU with a P.A. $=$ 145$^\circ$, and a dust mass of around 0.1 M$_\odot$. These physical parameters are in agreement with values obtained recently from millimeter observations. This submillimeter source is therefore related with the disk surrounding HL Tau.

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Alba M. Lumbreras, Luis A. Zapata. 2014-01-02. SMA Submillimeter Observations of HL Tau: Revealing a compact molecular outflow. https://doi.org/10.1088/0004-6256/147/4/72

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