Dust-Corrected Star Formation Rates of Galaxies. II. Combinations of Ultraviolet and Infrared Tracers

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

54 pages, 16 figures, accepted for publication in The Astrophysical Journal

Scientific paper

We present new calibrations of far-ultraviolet (FUV) attenuation as derived from the total infrared to FUV luminosity ratio (IRX) and the FUV-NUV color. We find that the IRX-corrected FUV luminosities are tightly and linearly correlated with the attenuation-corrected H\alpha\ luminosities (as measured from the Balmer decrement), with a rms scatter of $\pm 0.09$ dex. The ratios of these attenuation-corrected FUV to H\alpha\ luminosities are consistent with evolutionary synthesis model predictions, assuming a constant star formation rate over 100 Myr, solar metallicity and either a Salpeter or a Kroupa IMF with lower and upper mass limits of 0.1 and 100\msun. The IRX-corrected FUV to Balmer-corrected H\alpha\ luminosity ratios do not show any trend with other galactic properties over the ranges covered by our sample objects. In contrast, FUV attenuation derived from the FUV-NUV color (UV spectral slope) show much larger random and systematic uncertainties. When compared to either Balmer-corrected H\alpha\ luminosities or IRX-corrected FUV luminosities the color-corrected FUV luminosities show $\sim 2.5$ times larger rms scatter, and systematic nonlinear deviations as functions of luminosity and other parameters. Linear combinations of 25um and 1.4GHz radio continuum luminosities with the observed FUV luminosities are also well correlated with the Balmer-corrected H\alpha\ luminosities. These results provide useful prescriptions for deriving attenuation-corrected star formation rates of galaxies based on linear combinations of UV and IR or radio luminosities, which are presented in convenient tabular form. Comparisons of our calibrations with attenuation corrections in the literature and with dust attenuation laws are also made.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Dust-Corrected Star Formation Rates of Galaxies. II. Combinations of Ultraviolet and Infrared Tracers does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dust-Corrected Star Formation Rates of Galaxies. II. Combinations of Ultraviolet and Infrared Tracers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dust-Corrected Star Formation Rates of Galaxies. II. Combinations of Ultraviolet and Infrared Tracers will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-711863

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.