Constraining the Chemical Signatures and the Outburst Mechanism of the Class 0 Protostar HOPS 383
arXiv:2010.05939 · doi:10.3847/1538-4357/abbdf4
Abstract
We present observations toward HOPS 383, the first known outbursting Class 0 protostar located within the Orion molecular cloud using ALMA, VLA, and SMA. The SMA observations reveal envelope scale continuum and molecular line emission surrounding HOPS 383 at 0.85 mm, 1.1 mm, and 1.3 mm. The images show that HCO and HCO peaks on or near the continuum, while NH is reduced at the same position. This reflects the underlying chemistry where CO evaporating close to the protostar destroys NH while forming HCO. We also observe the molecular outflow traced by CO () and (). A disk is resolved in the ALMA 0.87 mm dust continuum, orthogonal to the outflow direction, with an apparent radius of 62 AU. Radiative transfer modeling of the continuum gives disk masses of 0.02 M when fit to the ALMA visibilities. The models including VLA 8 mm data indicate that the disk mass could be up to a factor of 10 larger due to lower dust opacity at longer wavelengths. The disk temperature and surface density profiles from the modeling, and an assumed protostar mass of 0.5 M suggest that the Toomre parameter before the outburst, making gravitational instability a viable mechanism to explain outbursts at an early age if the disk is sufficiently massive.
Accepted by ApJ
References in corpus (21)
- Cold Dark Clouds: The Initial Conditions for Star Formation
- The Burst Mode of Protostellar Accretion
- The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. A Statistical Characterization of Class 0 and I Protostellar Disks
- A Triple Protostar System Formed via Fragmentation of a Gravitationally Unstable Disk
- Experimental evidence for Glycolaldehyde and Ethylene Glycol formation by surface hydrogenation of CO molecules under dense molecular cloud conditions
- HOPS 383: An Outbursting Class 0 Protostar in Orion
- HH 212: SMA Observations of a Remarkable Protostellar Jet
- Molecule sublimation as a tracer of protostellar accretion: Evidence for accretion bursts from high angular resolution C18O images
- Chemical tracers of episodic accretion in low-mass protostars
- Chronology of Episodic Accretion in Protostars -- an ALMA survey of the CO and HO snowlines
- Disk Masses for Embedded Class I Protostars in the Taurus Molecular Cloud
- Constraining the Rate of Protostellar Accretion Outbursts in the Orion Molecular Clouds
- The chemistry of episodic accretion in embedded objects. 2D radiation thermo-chemical models of the post-burst phase
- Luminosity outburst chemistry in protoplanetary discs: going beyond standard tracers
- The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars I. Identifying and Characterizing the Protostellar Content of the OMC2-FIR4 and OMC2-FIR3 Regions
- The rotating molecular core and precessing outflow of the young stellar object Barnard 1c
- The CARMA-NRO Orion Survey: Protostellar Outflows, Energetics, and Filamentary Alignment
- The VLA Nascent Disk And Multiplicity Survey of Perseus Protostars (VANDAM). III. Extended Radio Emission from Protostars in Perseus
- Astro & cosmo-chemical consequences of accretion bursts I: the D/H ratio of water
- Constraining the Disk Masses of the Class I Binary Protostar GV Tau
- Evidence for magnetic activity at starbirth: a powerful X-ray flare from the Class 0 protostar HOPS 383
Cited by in corpus (5)
- The Rate, Amplitude and Duration of Outbursts from Class 0 Protostars in Orion
- Formation and evolution of protostellar accretion discs. I. Angular-momentum budget, gravitational self-regulation, and numerical convergence
- Early Planet Formation in Embedded Disks (eDisk) IX: High-resolution ALMA Observations of the Class 0 Protostar R CrA IRS5N and its surrounding
- Protostellar Outflows: a window to the past
- Early Planet Formation in Embedded Disks (eDisk). XX. Constraining the Chemical Tracers of Young Protostellar Sources