English

FAUST XII. Accretion streamers and jets in the VLA 1623--2417 protocluster

Solar and Stellar Astrophysics 2024-02-19 v1 Astrophysics of Galaxies

Abstract

The ALMA interferometer has played a key role in revealing a new component of the Sun-like star forming process: the molecular streamers, i.e. structures up to thousands of au long funneling material non-axisymmetrically to disks. In the context of the FAUST ALMA LP, the archetypical VLA1623-2417 protostellar cluster has been imaged at 1.3 mm in the SO(56_6--45_5), SO(66_6--55_5), and SiO(5--4) line emission at the spatial resolution of 50 au. We detect extended SO emission, peaking towards the A and B protostars. Emission blue-shifted down to 6.6 km s1^{-1} reveals for the first time a long (\sim 2000 au) accelerating streamer plausibly feeding the VLA1623 B protostar. Using SO, we derive for the first time an estimate of the excitation temperature of an accreting streamer: 33±\pm9 K. The SO column density is \sim 1014^{14} cm2^{-2}, and the SO/H2_2 abundance ratio is \sim 108^{-8}. The total mass of the streamer is 3 ×\times 103^{-3} MsunMsun, while its accretion rate is 3--5 ×\times 107^{-7} Msun yr1^{-1}. This is close to the mass accretion rate of VLA1623 B, in the 0.6--3 ×\times 107^{-7} Msun yr1^{-1} range, showing the importance of the streamer in contributing to the mass of protostellar disks. The highest blue- and red-shifted SO velocities behave as the SiO(5--4) emission, the latter species detected for the first time in VLA1623-2417: the emission is compact (100-200 au), and associated only with the B protostar. The SO excitation temperature is \sim 100 K, supporting the occurrence of shocks associated with the jet, traced by SiO.

Keywords

Cite

@article{arxiv.2402.10258,
  title  = {FAUST XII. Accretion streamers and jets in the VLA 1623--2417 protocluster},
  author = {C. Codella and L. Podio and M. De Simone and C. Ceccarelli and S. Ohashi and C. J. Chandler and N. Sakai and J. E. Pineda and D. M. Segura-Cox and E. Bianchi and N. Cuello and A. López-Sepulcre and D. Fedele and P. Caselli and S. Charnley and D. Johnstone and Z. E. Zhang and M. J. Maureira and Y. Zhang and G. Sabatini and B. Svoboda and I. Jiménez-Serra and L. Loinard and S. Mercimek and N. Murillo and S. Yamamoto},
  journal= {arXiv preprint arXiv:2402.10258},
  year   = {2024}
}

Comments

accepted by MNRAS