2008/06/25 by D. W. Weedman, Daniel W. Weedman, J. R. Houck +1 · 44 citations
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Galaxy #Infrared #Luminosity #Luminosity function #Luminous infrared galaxy #Physics #Star formation #astro-ph
paper · pdf · doi:10.1086/591123
published in The Astrophysical Journal 686(1), 127-137 (IOP Publishing) · Accepted for publication in The Astrophysical Journal
arxiv created 2008/06/25 · openalex publication_date 2008/10/07 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
A summary of starburst luminosities based on polycyclic aromatic hydrocarbon (PAH) features is given for 243 starburst galaxies with 0 < z < 2.5, observed with the Spitzer Infrared Spectrograph. Luminosity ν L ν (7.7 μm) for the peak luminosity of the 7.7 μm PAH emission feature is found to scale as log [ ν L ν (7.7 μm) ] = 44.63(± 0.09) + 2.48(± 0.28) log (1 + z) for the most luminous starbursts observed. Empirical calibrations of ν L ν (7.7 μm) are used to determine bolometric luminosity L IR and the star formation rate (SFR) for these starbursts. The most luminous starbursts found in this sample have log L IR = 45.4(± 0.3) + 2.5(± 0.3) log (1 + z) , in ergs s −1 , and the maximum star formation rates for starbursts in units of M ☉ yr −1 are log (SFR) = 2.1(± 0.3) + 2.5(± 0.3) log (1 + z) , up to z = 2.5. The exponent for pure luminosity evolution agrees with optical and radio studies of starbursts but is flatter than previous results based in infrared source counts. The maximum star formation rates are similar to the maxima determined for submillimeter galaxies; the most luminous individual starburst included within the sample has log L IR = 46.9, which gives an SFR = 3.4 × 10 3 M ☉ yr −1 .