The Effect of Metallicity on Cepheid Magnitudes and the Distance to M33

Victoria Scowcroft, David Bersier, Jeremy Mould, Peter Wood, Joyce Ann Guzik, Paul A. Bradley

Research output: Contribution to conferenceOther

1 Citation (Scopus)
Original languageEnglish
Pages43-47
DOIs
Publication statusPublished - 2009
EventStellar Pulsation: Challenges for Theory and Observation - Santa Fe, New Mexico, USA United States
Duration: 31 May 20095 Jun 2009

Conference

ConferenceStellar Pulsation: Challenges for Theory and Observation
CountryUSA United States
CitySanta Fe, New Mexico
Period31/05/095/06/09

Cite this

Scowcroft, V., Bersier, D., Mould, J., Wood, P., Guzik, J. A., & Bradley, P. A. (2009). The Effect of Metallicity on Cepheid Magnitudes and the Distance to M33. 43-47. Stellar Pulsation: Challenges for Theory and Observation, Santa Fe, New Mexico, USA United States. https://doi.org/10.1063/1.3246538

The Effect of Metallicity on Cepheid Magnitudes and the Distance to M33. / Scowcroft, Victoria; Bersier, David; Mould, Jeremy; Wood, Peter; Guzik, Joyce Ann; Bradley, Paul A.

2009. 43-47 Stellar Pulsation: Challenges for Theory and Observation, Santa Fe, New Mexico, USA United States.

Research output: Contribution to conferenceOther

Scowcroft, V, Bersier, D, Mould, J, Wood, P, Guzik, JA & Bradley, PA 2009, 'The Effect of Metallicity on Cepheid Magnitudes and the Distance to M33' Stellar Pulsation: Challenges for Theory and Observation, Santa Fe, New Mexico, USA United States, 31/05/09 - 5/06/09, pp. 43-47. https://doi.org/10.1063/1.3246538
Scowcroft V, Bersier D, Mould J, Wood P, Guzik JA, Bradley PA. The Effect of Metallicity on Cepheid Magnitudes and the Distance to M33. 2009. Stellar Pulsation: Challenges for Theory and Observation, Santa Fe, New Mexico, USA United States. https://doi.org/10.1063/1.3246538
Scowcroft, Victoria ; Bersier, David ; Mould, Jeremy ; Wood, Peter ; Guzik, Joyce Ann ; Bradley, Paul A. / The Effect of Metallicity on Cepheid Magnitudes and the Distance to M33. Stellar Pulsation: Challenges for Theory and Observation, Santa Fe, New Mexico, USA United States.
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