Star formation in M 33: multiwavelength signatures across the disk

2008/10/02 by S. Verley, E. Corbelli, C. Giovanardi +1 · 3 citations
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Star Formation Studies #Circumstellar disk #Infrared #Optics #Physics #Star (game theory) #Star formation #Stars #Stellar, planetary, and galactic studies #Ultraviolet #Wavelength #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810566

14 pages, 13 figures, 3 tables, accepted by A&A

arxiv created 2008/10/02 · openalex publication_date 2008/10/27 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims. We use different tracers, such as Hα, ultraviolet (UV), and infrared (IR) emissions at various wavelengths, to study the dust and star formation (SF) conditions throughout the disk of M 33.

Citations

• Photoelectric Emission from Interstellar Dust: Grain Charging and Gas Heating
• The size distribution of interstellar grains
• Star Formation in NGC 5194 (M51a): The Panchromatic View fromGALEXtoSpitzer
• Infrared Spectral Energy Distributions of Nearby Galaxies
• TheGalaxy Evolution Explorer: A Space Ultraviolet Survey Mission
• The Nature of Infrared Emission in the Local Group Dwarf Galaxy NGC 6822 as Revealed bySpitzer
• The Polycyclic Aromatic Hydrocarbon Emission Deficit in Low‐Metallicity Galaxies—ASpitzerView
• The M33 Metallicity Project: Resolving the Abundance Gradient Discrepancies in M33
• Starburst99: Synthesis Models for Galaxies with Active Star Formation
• The Spitzer Space Telescope Mission
• Evolution of Asymptotic Giant Branch Stars
• STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE
• Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 M_\odot, and from Z=0.0004 to 0.03

Cited by

• Dynamical signatures of a ΛCDM-halo and the distribution of the baryons in M 33
• Galaxy And Mass Assembly (GAMA): the life and times of L★ galaxies
• Modeling the total and polarized emission in evolving galaxies: “Spotty” magnetic structures