Infall/Expansion Velocities in the Low-Mass Dense Cores L492, L694-2, and L1521F: Dependence on Position and Molecular Tracer

Abstract

Although surveys of infall motions in dense cores have been carried out for years, few surveys have focused on mapping infall across cores using multiple spectral line observations. To fill this gap, we present IRAM 30-m Telescope maps of N2H+(1-0), DCO+(2-1), DCO+(3-2), and HCO+(3-2) emission towards two prestellar cores (L492 and L694-2) and one protostellar core (L1521F). We find that the measured infall velocity varies with position across each core and choice of molecular line, likely as a result of radial variations in core chemistry and dynamics. Line-of-sight infall speeds estimated from DCO+(2-1) line profiles can decrease by 40-50 m/s when observing at a radial offset >= 0.04 pc from the core's dust continuum emission peak. Median infall speeds calculated from all observed positions across a core can also vary by as much as 65 m/s depending on the transition. These results show that while single-pointing, single-transition surveys of core infall velocities may be good indicators of whether a core is either contracting or expanding, the magnitude of the velocities they measure are significantly impacted by the choice of molecular line, proximity to the core center, and core evolutionary state.

Accepted for publication in ApJ

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Cited by in corpus (10)

• A large (~1 pc) contracting envelope around the prestellar core L1544
• First detection of CHD${}_2$OH towards pre-stellar cores
• Parsec-scale cosmic-ray ionisation rate in Orion
• Role of Filamentary Structures in the Formation of Two Dense Cores, L1544 and L694-2
• Gas infalling motions in the envelopes of Very Low Luminosity Objects
• A Catalog of Molecular Clumps and Cores with Infall Signatures
• A particular carbon-chain-producing region: L1489 starless core
• Carbon-chain molecule survey toward four low-mass molecular outflow sources
• Cosmic-ray ionisation rate in low-mass cores: the role of the environment
• Studying Infall in Infrared Dark Clouds with Multiple HCO+ Transitions