24–26 Jun 2025
Istanbul Technical University
Europe/Istanbul timezone

The TRGB-SBF Project: a Pop II path to H0

24 Jun 2025, 11:10
40m
Istanbul Technical University

Istanbul Technical University

İTÜ Ayazağa Campus, Rectorate Building, 34469 Maslak-ISTANBUL Phone:+90 212 285 30 30

Speaker

Brent Tully (University of Hawaii)

Description

The path from Cepheid variables to type Ia supernovae gives a value of the Hubble constant which significantly disagrees with the value determined from observations of conditions in the early universe and a cosmological model. A totally independent measurement of H0 from observed redshifts and distances is needed to evaluate the possibilities of systematic errors. A path is being explored that should be as accurate or better than the Cepheid-SNIa way, involving only observations of old evolved stars. Gaia parallaxes ground the absolute values of RR Lyrae stars that establish the absolute magnitudes of stars at the tip of the red giant branch that sets the scale of the power spectrum of surface brightness fluctuations in E/S0 galaxies that are observed with negligible confusion from peculiar velocities. Observations with JWST are fundamental for the success of this program.

Primary author

Brent Tully (University of Hawaii)

Presentation materials

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