A Case Study of Low-Mass Star Formation

Abstract

This article synthesizes observational data from an extensive program aimed toward a comprehensive understanding of star formation in a low-mass star-forming molecular cloud. New observations and published data spanning from the centimeter wave band to the near infrared reveal the high and low density molecular gas, dust, and pre-main sequence stars in L1551.

24 pages, 21 figures, ApJS accepted

References in corpus (9)

• Slow Star Formation in Dense Gas: Evidence and Implications
• Equilibrium Star Cluster Formation
• Cluster Formation in Protostellar Outflow-Driven Turbulence
• Velocity centroids as tracers of the turbulent velocity statistics
• Star Formation in Space and Time: The Orion Nebula Cluster
• Multi-Generational Star Formation in L1551
• Entrainment Mechanisms for Outflows in the L1551 Star-Forming Region
• Outflow Driven Cavities: Numerical Simulations of Intermediaries of Protostellar Turbulence
• Short Spacing Synthesis from a Primary Beam Scanned Interferometer

Cited by in corpus (36)

• Outflow Feedback Regulated Massive Star Formation in Parsec-Scale Cluster Forming Clumps
• Modeling jet and outflow feedback during star cluster formation
• Turbulent Driving Scales in Molecular Clouds
• The Turbulent Warm Ionized Medium: Emission Measure Distribution and MHD Simulations
• Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars
• Obtaining Spectra of Turbulent Velocity from Observations
• Impact of Protostellar Outflows on Turbulence and Star Formation Efficiency in Magnetized Dense Cores
• Feedback Effects on Low-Mass Star Formation
• Investigations of Protostellar Outflow Launching and Gas Entrainment: Hydrodynamic Simulations and Molecular Emission
• The Age, Stellar Content and Star Formation Timescale of the B59 Dense Core
• Constraining the Envelope Structure of L1527 IRS: Infrared Scattered Light Modeling
• Radiation-Hydrodynamic Simulations of Protostellar Outflows: Synthetic Observations and Data Comparisons
• The HI-to-H2 Transition in a Turbulent Medium
• Observing Simulated Protostars with Outflows: How Accurate are Protostellar Properties Inferred from SEDs?
• Physical Properties of Dense Cores in the Rho Ophiuchi Main Cloud and A Significant Role of External Pressures in Clustered Star Formation
• Confronting Outflow-Regulated Cluster Formation Model with Observations
• Impact of Winds from Intermediate-Mass Stars on Molecular Cloud Structure and Turbulence
• Assessing molecular outflows and turbulence in the protostellar cluster Serpens South
• The Dynamics of the Envelope Surrounding the Protostar HH 211-mm
• Low-mass protostars and dense cores in different evolutionary stages in IRAS 00213+6530
• Tracing magnetic field morphology using the Velocity Gradient Technique in the presence of CO self-absorption
• Diverse protostellar evolutionary states in the young cluster AFGL961
• Early phase of massive star formation: A case study of Infrared dark cloud G084.81-01.09
• Nature of Striation in 21 cm Channel Maps: Velocity Caustics
• An Exploration of the Statistical Signatures of Stellar Feedback
• Propagation of Highly Efficient Star Formation in NGC 7000
• Near-infrared polarimetry of a normal spiral galaxy viewed through the Taurus Molecular Cloud Complex
• Cold Dust in Hot Regions
• The CARMA-NRO Orion Survey: Statistical Signatures of Feedback in the Orion A Molecular Cloud
• The Spatial Power Spectrum and Derived Turbulent Properties of Isolated Galaxies
• Probing the Physics of Star-Formation (ProPStar) III. No evidence for dissipation of turbulence down to 20 mpc (4 000 au) scale
• Molecular gas properties in young stellar clusters with a suppressed star cluster wind
• Turbulent Action at a Distance due to Stellar Feedback in Magnetized Clouds
• Identification of Anomalous E+A Galaxies in GAMA Using an Isolation Forest
• Characterizing Outflows in the Cygnus X Region
• Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies