'Star formation rate sfr' presentation slideshows

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H OPCAT , 6dFGS & Star Formation Rates

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H OPCAT , 6dFGS & Star Formation Rates

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H OPCAT , 6dFGS & Star Formation Rates

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X-ray luminosity evolution of XRBs in normal galaxies

X-ray luminosity evolution of XRBs in normal galaxies. Zhaoyu Zuo 2009-03-18. aim. To study how the X-ray properties of late-type field galaxies evolve as a function of optical luminosity , stellar mass , and star formation rate (SFR) with time. Observations.

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Galactic and Extragalactic star formation

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We investigated these for a sample of late-type,

It is well known that the H ? luminosity is a good tracer of the star formation in a galaxy (Kennicutt 1983 ApJ, 273, 54). The Star Formation Rate (SFR) along the Hubble sequence has been studied extensively (e.g. Kennicutt 1998 ARA&A, 36, 189) and some of the main results are:

109 views • 1 slides