HH 223: a parsec-scale H2outflow in the star-forming region L723
R. García López, Jose Antonio Acosta-Pulido, Gérard Gómez, R. Estalella, Carlos Carrasco‐González
Abstract
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R. García López, Jose Antonio Acosta-Pulido, Gérard Gómez, R. Estalella, Carlos Carrasco‐González
Abstract
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Context. The dark cloud Lynds 723 (L723) is a low-mass star-forming region where one of the few known cases of a quadrupolar CO outflow has been reported. Two recent works have found that the radio continuum source VLA 2, towards the centre of the CO outflow, is actually a multiple system of young stellar objects (YSOs). Several line-emission nebulae that lie projected on the east-west CO outflow were detected in narrow-band Hα and [S ii] images. The spectra of the knots are characteristic of shock-excited gas (Herbig-Haro spectra), with supersonic blueshifted velocities, which suggests an optical outflow also powered by the VLA 2 YSO system of L723.
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Context. The dark cloud Lynds 723 (L723) is a low-mass star-forming region where one of the few known cases of a quadrupolar CO outflow has been reported. Two recent works have found that the radio continuum source VLA 2, towards the centre of the CO outflow, is actually a multiple system of young stellar objects (YSOs). Several line-emission nebulae that lie projected on the east-west CO outflow were detected in narrow-band Hα and [S ii] images. The spectra of the knots are characteristic of shock-excited gas (Herbig-Haro spectra), with supersonic blueshifted velocities, which suggests an optical outflow also powered by the VLA 2 YSO system of L723.
Key concepts: Outflow, Astrophysics, Herbig–Haro object, Physics, Young stellar object, Spectral line, Emission spectrum, Supersonic speed