Michael Strauss

30.06.2013 • Views

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Michael Strauss

Michael Strauss

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The relative number of Type I and Type II galaxies<br />

is a function of luminosity

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What is different about LINER Galaxies

Stephen Murray - Astronomy and Astrophysics - University of ...

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Seyfert I galaxies are recognized by their broad permitted emission lines. The distribution of line widths is strongly bimodal.

The relative number of Type I and Type II galaxies is a function of luminosity

Page 1 and 2: Nearly Normal Active Galactic Nucle
Page 3 and 4: Using SDSS for AGN Studies n A colo
Page 5 and 6: The Luminosity Function from the fu
Page 7 and 8: Comoving number density peaks betwe
Page 9 and 10: The nature of low-luminosity quasar
Page 11: Ratios of various emission lines al
Page 15 and 16: n Very few high-luminosity Type II
Page 17 and 18: How do we determine intrinsic lumin
Page 19 and 20: • Multiband continuum imaging wit
Page 21 and 22: A montage of HST images of SDSSSDSS
Page 23 and 24: These objects have IRAC colors cons
Page 25 and 26: 19 quasars with z>5.7