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Towards observations of Population III galaxies

Published online by Cambridge University Press:  26 May 2016

Daniel Schaerer
Affiliation:
Laboratoire d'Astrophysique, Observatoire de Midi-Pyrénées, 14 Avenue E. Belin, F-31400 Toulouse, la France
Roser Pelló
Affiliation:
Laboratoire d'Astrophysique, Observatoire de Midi-Pyrénées, 14 Avenue E. Belin, F-31400 Toulouse, la France

Extract

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We are undertaking various studies of primordial galaxies with the following main aims:

  1. (i) synthesize the properties of rest-frame UV-optical spectra of Population III galaxies and ‘transition objects’ between Pop III and normal starbursts;

  2. (ii) devise optimal search strategies for the detection of Pop III and related objects with ground-based and space observations;

  3. (iii) simulate photometric and spectroscopic observations of Pop III galaxies to quantify the feasibility of such studies especially for future ground-based instruments; and

  4. (iv) study the physics of Pop III and ‘transition’ galaxies and their implications on cosmology and the physics of galaxies

Type
Part 4. Feedback from Massive Stars
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Malhotra, S., Rhoads, J.E. 2002, ApJ (Letters) 565, L7.Google Scholar
Schaerer, D. 2002, A&A 382, 28.Google Scholar
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Schaerer, D., Pelló, R. 2002a, in: Bergeron, J. & Monnet, G. (eds.), Scientific Drivers for ESO Future VLT/VLTI Instrumentation, ESO Astrophysics Symposia (Berlin: Springer), p. 48.Google Scholar
Schaerer, D., Pelló, R. 2002b, in: Sauvage, M., Stasinska, G., Vigroux, L., Schaerer, D. & Madden, S. (eds.), The Evolution of Galaxies. II. Basic Building Blocks, Ap&SS 281, 475.Google Scholar
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