The WFC3 Galactic bulge treasury program: Metallicity estimates for the stellar population and exoplanet hosts

Thomas M. Brown, Kailash Sahu, Jay Anderson, Jason Tumlinson, Jeff A. Valenti, Ed Smith, Elizabeth J. Jeffery, Alvio Renzini, Manuela Zoccali, Henry C. Ferguson, Don A. VandenBerg, Howard E. Bond, Stefano Casertano, Elena Valenti, Dante Minniti, Mario Livio, Nino Panagia

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

39 Citas (Scopus)

Resumen

We present new UV-to-IR stellar photometry of four low-extinction windows in the Galactic bulge, obtained with the Wide Field Camera 3 on the Hubble Space Telescope (HST). Using our five bandpasses we have defined reddening-free photometric indices sensitive to stellar effective temperature and metallicity. We find that the bulge populations resemble those formed via classical dissipative collapse: each field is dominated by an old (∼10 Gyr) population exhibiting a wide metallicity range (-1.5 ≲ [Fe/H] ≲ 0.5). We detect a metallicity gradient in the bulge population, with the fraction of stars at super-solar metallicities dropping from 41% to 35% over distances from the Galactic center ranging from 0.3 to 1.2 kpc. One field includes candidate exoplanet hosts discovered in the SWEEPS HST transit survey. Our measurements for 11 of these hosts demonstrate that exoplanets in the distinct bulge environment are preferentially found around high-metallicity stars, as in the solar neighborhood, supporting the view that planets form more readily in metal-rich environments.

Idioma originalInglés
Páginas (desde-hasta)L19-L23
PublicaciónAstrophysical Journal Letters
Volumen725
N.º1 PART 2
DOI
EstadoPublicada - 10 dic 2010

Áreas temáticas de ASJC Scopus

  • Astronomía y astrofísica
  • Ciencias planetarias y espacial

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