Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-12-02T21:57:42.142Z Has data issue: false hasContentIssue false

Can the first stars formed be pre-galactic?

Published online by Cambridge University Press:  07 August 2017

J. C. N. de Araujo
Affiliation:
Instituto Astronômico e Geofísico - U.S.P. C.P. 9638, 01065 SÃo Paulo, S.P. - Brasil
R. Opher
Affiliation:
Instituto Astronômico e Geofísico - U.S.P. C.P. 9638, 01065 SÃo Paulo, S.P. - Brasil

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We show that in a scenario of isothermal density perturbations, stars ≥50M (Population III) at a redshift z ≫ zgal (redshift of galaxy formation) can be formed. We take into account in the calculation the expansion of the Universe and a series of physical processes relevant to the primordial plasma: photon-drag, photon-cooling, recombination, collisional ionization, photoionization, Lyman-α cooling and molecular hydrogen cooling.

Type
Poster Papers
Copyright
Copyright © Kluwer 

References

de Araujo, J. C. N. & Opher, R. 1988, MNRAS, 231, 923.Google Scholar
de Araujo, J. C. N. & Opher, R. 1989, MNRAS, 239, 271.Google Scholar
de Araujo, J. C. N. & Opher, R. 1991, ApJ (in press).Google Scholar
Hogan, C. 1978, MNRAS, 185, 889.Google Scholar
Lahav, O. 1986, MNRAS, 220, 259.Google Scholar