Young Super Star Clusters in the Starburst of M82: The Catalogue
arXiv:astro-ph/0409750 · doi:10.1086/426421
Abstract
Recent results from Hubble Space Telescope (HST) have resolved starbursts as collections of compact young stellar clusters. Here we present a photometric catalogue of the young stellar clusters in the nuclear starburst of M82, observed with the HST WFPC2 in Halpha (F656N) and in four optical broad-band filters. We identify 197 young super stellar clusters. The compactness and high density of the sources led us to develop specific techniques to measure their sizes. Strong extinction lanes divide the starburst into five different zones and we provide a catalogue of young super star clusters for each of these. In the catalogue we include relative coordinates, radii, fluxes, luminosities, masses, equivalent widths, extinctions, and other parameters. Extinction values have been derived from the broad-band images. The radii range between 3 and 9 pc, with a mean value of 5.7 +/- 1.4pc, and a stellar mass between 10e4 and 10e6 Mo. The inferred masses and mean separation, comparable to the size of super star clusters, together with their high volume density, provides strong evidence for the key ingredients postulated by Tenorio et al. (2003) as required for the development of a supergalactic wind.
45 pages, 5 figures, 12 tables. Accepted for publication in ApJ. Added Erratum
References in corpus (1)
Cited by in corpus (59)
- The Disruption of Giant Molecular Clouds by Radiation Pressure and the Efficiency of Star Formation in Galaxies
- Supernova feedback efficiency and mass loading in the starburst and galactic superwind exemplar M82
- A connection between star formation activity and cosmic rays in the starburst galaxy M 82
- Super star clusters in Haro 11: Properties of a very young starburst and evidence for a near-infrared flux excess
- HST/STIS Spectroscopy of Five Super Star Clusters in the Starburst Galaxy M82
- SPIRE imaging of M82: cool dust in the wind and tidal streams
- Spectroscopic FIR mapping of the disk and galactic wind of M82 with Herschel-PACS
- Submillimeter-HCN Diagram for an Energy Diagnostics in the Centers of Galaxies
- The optical structure of the starburst galaxy M82 - I: Dynamics of the disk and inner-wind
- Two Populations of Molecular Clouds in the Antennae Galaxies
- The Optical Structure of the Starburst Galaxy M82. II. Nebular Properties of the Disk and Inner-Wind
- Deep MERLIN 5GHz Radio Imaging of Supernova Remnants in the M82 Starburst
- Two-Dimensional Hydrodynamic Models of Super Star Clusters with a Positive Star Formation Feedback
- Massive Clumps in Local Galaxies: Comparisons with High-Redshift Clumps
- M82, Starbursts, Star Clusters, and the Formation of Globular Clusters
- Effects of Galactic fountains and delayed mixing in the chemical evolution of the Milky Way
- A spectroscopic census of the M82 stellar cluster population
- HST/STIS spectroscopy of the environment in the starburst core of M82
- Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations
- On the chemistry and distribution of HOC+ in M82: More evidence for extensive PDRs
- On the feedback from super stellar clusters. I. The structure of giant HII regions and HII galaxies
- Evolution of Super Star Cluster Winds with Strong Cooling
- The formation of secondary stellar generations in massive young star clusters from rapidly cooling shocked stellar winds
- HST/ACS imaging of M82: A comparison of mass and size distribution functions of the younger nuclear and older disk clusters
- The pressure confined wind of the massive and compact superstar cluster M82-A1
- Interpreting the Low Frequency Radio Spectra of Starburst Galaxies: A Pudding of Strömgren Spheres
- Initial Populations of Black Holes in Star Clusters
- On the Extreme Positive Feedback Star-Forming Mode from Massive and Compact Superstar Clusters
- The Star Cluster System in the Nearby Starburst Galaxy M82
- Search for Tidal Dwarf Galaxies Candidates in a Sample of Ultraluminous Infrared Galaxies
- Star cluster versus field star formation in the nucleus of the prototype starburst galaxy M82
- Short Hard Gamma Ray Bursts And Their Afterglows
- The Global Star-Formation Law by Supernova Feedback
- Winds from clu\sters with non-uniform stellar distributions
- Star Cluster Complexes and the Host Galaxy in Three HII Galaxies: Mrk 36, UM 408, and UM 461
- Detection of additional Wolf-Rayet stars in the starburst cluster Westerlund 1 with SOAR
- Galaxy Collisions - Dawn of a New Era
- On the Heating Efficiency Derived from Observations of Young Super Star Clusters in M82
- The Complex North Transition Region of Centaurus A: Radio Structure
- Diffuse Thermal X-Ray Emission in the Core of the Young Massive Cluster Westerlund 1
- Hubble Space Telescope Observations of Accretion-Induced Star Formation in the Tadpole Galaxy Kiso 5639
- Spatially Resolved Star Formation History Along the Disk of M82 Using Multi-Band Photometric Data
- A High Resolution Map of 12CO J=6-5 Emission in the Starburst Galaxy M82
- Filaments in Galactic Winds Driven by Young Stellar Clusters
- Locating the Youngest HII Regions in M82 with 7 mm Continuum Maps
- Star Formation History of a Young Super-Star Cluster in NGC 4038/39: Direct Detection of Low Mass Pre-Main Sequence Stars
- On the X-ray emission from massive star clusters and their evolving superbubbles II. Detailed analytics and observational effects
- On the thermal structure of the proto-Super Star Cluster 13 in NGC 253
- Star cluster disruption in the starburst galaxy Messier 82
- Structural analysis of disk super star clusters of M82: size and profile shape at intermediate ages
- Evolving Starburst Modeling of FIR/sub-mm/mm Line Emission. II. Application to M 82
- Low and high velocity clouds produced by young stellar clusters
- Could the Compact Radio Sources in M82 be Cluster Wind Driven Bubbles?
- Hot Gas Outflow Properties of the Starburst Galaxy NGC 4945
- SDSSJ103913.70+533029.7: A Super Star Cluster in the Outskirts of a Galaxy Merger
- Mass and metal ejection efficiency in disk galaxies driven by young stellar clusters of nuclear starburst
- Catastrophic Cooling in Superwinds. II. Exploring the Parameter Space
- Optical/Near-IR spatially resolved study of the H II galaxy Tol 02
- Evolving Starburst Modeling of FIR/sub-mm/mm Line Emission. III. Application to Nearby Luminous Infrared Galaxies