What We Can Learn from the Light Curves of GD 358 and PG 1351+489

Details What We Can Learn from the Light Curves of GD 358 and PG 1351+489 What We Can Learn from the Light Curves of GD 358 and PG 1351+489

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.154...38m&link_type=abstract

Communications in Asteroseismology, Vol. 154, p.38-48

Physics

8

Scientific paper

We present the results of light curve fits to two DBV white dwarfs, PG 1351+489 and GD 358. For both fits, we include recent improvements in calculations relating the bolometric and observed flux variations. We provide a preliminary map of convection across the DB instability strip, and we show how this allows us to choose between two possible spectroscopic fits to PG 1351+489.

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