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Magnetic White Dwarfs in SDSS Estimating the Mean Mass of Normal DAs and DBs

Magnetic White Dwarfs in SDSS Estimating the Mean Mass of Normal DAs and DBs . Kepler Scot Kleinman , Atsuko Nitta B árbara Castanheira, Detlev Koester Marcos Diaz . H b. H a. Analysis of hydrogen-rich magnetic white dwarfs detected in the Sloan Digital Sky Survey

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Magnetic White Dwarfs in SDSS Estimating the Mean Mass of Normal DAs and DBs

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  1. Magnetic White Dwarfs in SDSS Estimating the Mean Mass of Normal DAs and DBs Kepler Scot Kleinman, Atsuko Nitta Bárbara Castanheira, Detlev Koester Marcos Diaz

  2. Hb Ha

  3. Analysis of hydrogen-rich magnetic white dwarfs detected in the Sloan Digital Sky Survey BaybarsKülebi, Stefan Jordan, Fabian Euchner, Boris Gänsicke & Heiko Hirsch 2009 -model the structure of the surface magnetic fields of the hydrogen-rich white dwarfs in the SDSS, -analysedthe spectra of all known magnetic DAs from the SDSS : 97 previously published plus 44 newly discovered.

  4. Estimated “log g”

  5. Mass > 1.1 Mo white dwarfs

  6. dM SDSS J121105.25-004628.5 0287-253-52023 DAH S/N=14 Teff=22490+371K, log g=9.06+0.06

  7. B>1 MG 755 DAH and 12549 DA, 5.7% 62 DBH and 889 DB, 6.5% 937+767 DH in 19503WD, 4.8%+3.9 B<1 MG <M>=0.605+0.004 Msun, DAs, S/N>25, Teff>12000K, <S/N>=35, N=991 <M>=0.645+0.006 Msun, DBs, S/N>25, Teff>16000K, <S/N>=32, N=43 DBs, S/N>25, 1:3:18 for Teff>45000K:30000K:20000K exactly what expected by age -> NO DB GAP! -A Spectroscopic Analysis of White Dwarfs in the Kiso Survey M.-M. Limoges and P. Bergeron 2010 0.606 Msun and a dispersion of 0.135 M for 149 DAs 0.758 Msun and a dispersion of 0.192 M for 19 DBs -Spectroscopic Analysis of DA WD: Stark Broadening of H including non-ideal effects P.-E. Tremblay and P. Bergeron 2009 0.649 Msunfor 250 DAs

  8. Emission lines Aurora 10-16 Mo

  9. Aurora? 10-16 Mo

  10. Same star!

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