Abstract
We report molecular line observations of CO(1-0), <TEX>$^{13}CO(1-0)$</TEX>, CS(2-1), and HCN(1-0) with SRAO 6m telescope toward L1014-IRS which is thought to be a very faint infrared source embedded in previously known 'starless' core L1014. The CO(1-0) observations find several components with different velocities along the line of sight of L1014, <TEX>$4km\;s^{-1}$</TEX> and between <TEX>$40{\sim}50km\;s^{-1}$</TEX>. We find a parsec scale CO molecular outflow at the <TEX>$4km\;s^{-1}$</TEX> component for the first time the direction of which is coincident with that of the small scale (<TEX>${\sim}500pc$</TEX>) outflow previously found. Although the observation is not covered for whole area of the outflow, the size of the molecular outflow seems not very inconsistent with the expected age of L1014-IRS. More accurate size and shape of the molecular outflow from L1014-IRS will be determined from the full coverage mapping in CO over the outflow region in very near future.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
