1. Bipolar molecular outflow of the very low-mass star Par-Lup3-4: Evidence for scaled-down low-mass star formation
- Author
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F. Comerón, Matthias R. Schreiber, A. Santamaria-Miranda, A. Ribas, Koraljka Mužić, Nuria Huélamo, I. de Gregorio-Monsalvo, Leonardo Testi, C. Lopez, Adele Plunkett, Unidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737, Agencia Estatal de Investigación (AEI), Santamaría Miranda, A. [0000-0001-6267-2820], De Gregorio Monsalvo, I. [0000-0003-4518-407X], Huélamo, N. [0000-0002-2711-8143], Plunkett, A. [0000-0002-9912-5705], Comerón, F. [0000-0002-7838-2606], Schreiber, M. [0000-0003-3903-8009], Muzic, K. [0000-0002-7989-2595], Testi, L. [0000-0003-1859-3070], and Spanish State Research Agency MCIU/AEI (Spain)
- Subjects
Physics ,010308 nuclear & particles physics ,Star formation ,jets and outflows [ISM] ,Astrophysics::High Energy Astrophysical Phenomena ,Astronomy and Astrophysics ,individual objects [ISM] ,stars [Submillimeter] ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Star (graph theory) ,01 natural sciences ,Space and Planetary Science ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Par-Lup3-4 ,interferometric [Techniques] ,Outflow ,Low Mass ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,formation [Stars] - Abstract
Context. Very low-mass stars are known to have jets and outflows, which is indicative of a scaled-down version of low-mass star formation. However, only very few outflows in very low-mass sources are well characterized. Aims. We characterize the bipolar molecular outflow of the very low-mass star Par-Lup3-4, a 0.12 M object known to power an optical jet. Methods. We observed Par-Lup3-4 with ALMA in Bands 6 and 7, detecting both the continuum and CO molecular gas. In particular, we studied three main emission lines: CO(2-1), CO(3-2), and 13 CO(3-2). Results. Our observations reveal for the first time the base of a bipolar molecular outflow in a very low-mass star, as well as a stream of material moving perpendicular to the primary outflow of this source. The primary outflow morphology is consistent with the previously determined jet orientation and disk inclination. The outflow mass is 9.5 × 10 -7 M , with an outflow rate of 4.3 × 10 -9 M yr -1 . A new fitting to the spectral energy distribution suggests that Par-Lup3-4 may be a binary system. Conclusions. We have characterized Par-Lup3-4 in detail, and its properties are consistent with those reported in other very low-mass sources. This source provides further evidence that very low-mass sources form as a scaled-down version of low-mass stars., With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737)
- Published
- 2020