H Morphologies of Star Clusters: A LEGUS study of HII region evolution timescales and stochasticity in low mass clusters
arXiv:1910.02983 · doi:10.1093/mnras/stz2820
Abstract
The morphology of HII regions around young star clusters provides insight into the timescales and physical processes that clear a cluster's natal gas. We study ~700 young clusters (<10Myr) in three nearby spiral galaxies (NGC 7793, NGC 4395, and NGC 1313) using Hubble Space Telescope (HST) imaging from LEGUS (Legacy ExtraGalactic Ultraviolet Survey). Clusters are classified by their H morphology (concentrated, partially exposed, no-emission) and whether they have neighboring clusters (which could affect the clearing timescales). Through visual inspection of the HST images, and analysis of ages, reddenings, and stellar masses from spectral energy distributions fitting, together with the (U-B), (V-I) colors, we find: 1) the median ages indicate a progression from concentrated (~3 Myr), to partially exposed (~4 Myr), to no H emission (>5Myr), consistent with the expected temporal evolution of HII regions and previous results. However, 2) similarities in the age distributions for clusters with concentrated and partially exposed H morphologies imply a short timescale for gas clearing (<1Myr). 3) our cluster sample's median mass is ~1000 M, and a significant fraction (~20%) contain one or more bright red sources (presumably supergiants), which can mimic reddening effects. Finally, 4) the median E(B-V) values for clusters with concentrated H and those without H emission appear to be more similar than expected (~0.18 vs. ~0.14, respectively), but when accounting for stochastic effects, clusters without H emission are less reddened. To mitigate stochastic effects, we experiment with synthesizing more massive clusters by stacking fluxes of clusters within each H morphological class. Composite isolated clusters also reveal a color and age progression for H morphological classes, consistent with analysis of the individual clusters.
20 pages, 16 figures, 7 tables; accepted for publication in MNRAS
References in corpus (6)
- Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback
- Legacy ExtraGalactic UV Survey (LEGUS) with The Hubble Space Telescope. I. Survey Description
- Studying the YMC population of M83: how long clusters remain embedded, their interaction with the ISM and implications for GC formation theories
- Using H-alpha Morphology and Surface Brightness Fluctuations to Age-Date Star Clusters in M83
- Age, size, and position of H ii regions in the Galaxy. Expansion of ionized gas in turbulent molecular clouds
- Star Cluster Catalogs for the LEGUS Dwarf Galaxies
Cited by in corpus (45)
- The lifecycle of molecular clouds in nearby star-forming disc galaxies
- The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular resolution in Nearby GalaxieS
- The molecular cloud lifecycle
- The GRIFFIN project -- Formation of star clusters with individual massive stars in a simulated dwarf galaxy starburst
- PHANGS-JWST First Results: Multi-wavelength view of feedback-driven bubbles (The Phantom Voids) across NGC 628
- PHANGS-HST: Star Cluster Spectral Energy Distribution Fitting with CIGALE
- The impact of pre-supernova feedback and its dependence on environment
- LEGUS and Halpha-LEGUS Observations of Star Clusters in NGC 4449: Improved Ages and the Fraction of Light in Clusters as a Function of Age
- Star Cluster Classification in the PHANGS-HST Survey: Comparison between Human and Machine Learning Approaches
- PHANGS-HST: New Methods for Star Cluster Identification in Nearby Galaxies
- Momentum feedback from marginally-resolved HII regions in isolated disc galaxies
- PHANGS-JWST First Results: Duration of the early phase of massive star formation in NGC628
- H Morphologies of Star Clusters in 16 LEGUS Galaxies: Constraints on HII region evolution timescales
- Quantifying the energetics of molecular superbubbles in PHANGS galaxies
- Stellar feedback in M83 as observed with MUSE -- II. Analysis of the HII region population: ionisation budget and pre-SN feedback
- Looking for obscured young star clusters in NCG 1313
- Linking stellar populations to HII regions across nearby galaxies: I. Constraining pre-supernova feedback from young clusters in NGC1672
- The formation of massive stellar clusters in converging galactic flows with photoionisation
- Bright, Relatively Isolated Star Clusters in PHANGS-HST Galaxies: Aperture Corrections, Quantitative Morphologies, and Comparison with Synthetic Stellar Population Models
- Improving Star Cluster Age Estimates in PHANGS-HST Galaxies and the Impact on Cluster Demographics in NGC 628
- Stellar associations powering HII regions $\unicode{x2013}$ I. Defining an evolutionary sequence
- Embedded Young Massive Star Clusters in the Antennae Merger
- Revisiting Attenuation Curves: the Case of NGC 3351
- Multi-Scale Stellar Associations across the Star Formation Hierarchy in PHANGS-HST Nearby Galaxies: Methodology and Properties
- The Dependence of the Hierarchical Distribution of Star Clusters on Galactic Environment
- Star Cluster Classification using Deep Transfer Learning with PHANGS-HST
- The SOFIA FEEDBACK Legacy Survey: Rapid molecular cloud dispersal in RCW 79
- Candidate LBV stars in galaxy NGC 7793 found via HST photometry + MUSE spectroscopy
- The loss of the intra-cluster medium in globular clusters
- Synthetic photometry of OB star clusters with stochastically sampled IMFs: analysis of models and HST observations
- Empirical SED Templates for Star Clusters Observed with HST and JWST: No Strong PAH or IR Dust Emission after Five Myr
- Spectroscopy of CASSOWARY gravitationally-lensed galaxies in SDSS: characterisation of an extremely bright reionization-era analog at
- The Timescales of Star Cluster Emergence: The Case of NGC 4449
- GOALS-JWST: NIRCam and MIRI Imaging of the Circumnuclear Starburst Ring in NGC 7469
- Dust Buried Compact Sources in the Dwarf Galaxy NGC 4449
- Constraining the LyC escape fraction from LEGUS star clusters with SIGNALS HII region observations: A pilot study of NGC 628
- HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations
- Simulations of pre-supernova feedback in spherical clouds
- Observing the Earliest Stages of Star Formation in Galaxies: 8 micron Cores in Three Edge-on Disks
- Constraining the top-light initial mass function in the extended ultraviolet disk of M83
- Duration and properties of the embedded phase of star formation in 37 nearby galaxies from PHANGS-JWST
- The Star Formation Factory revisited I. The impact of metallicity on collapsing star-forming clouds
- Studying the ISM at 10 pc scale in NGC 7793 with MUSE -- II. Constraints on the oxygen abundance and ionising radiation escape
- Stellar associations powering HII regions $\unicode{x2013}$ II. Escape fraction of ionizing photons
- Kinematics and Feedback in H II regions in the Dwarf Starburst Galaxy IC 10