---
res:
  bibo_abstract:
  - With the help of numerical simulations, we examine two aspects of feedback from
    the first generation of stars on later star formation. First, we investigate the
    impact of relic HII regions on forming halos. We find that the positive and negative
    effects of such feedback nearly cancel because the increase in entropy due to
    heating is balanced by the increase in the H 2 fraction due to the free electrons.
    However, these halos can be delayed more easily by a background Lyman-Werner flux.
    Second, we show that HD cooling is important in halos which have been ionized
    and allowed to recombine. Gas is allowed to cool to the CMB temperature at densities
    around n∼10 4cm-3, reducing the accreted mass by a factor of a few. However, as
    the collapse proceeds, the central gas density exceeds the critical density of
    HD and heats until HD cooling is no longer important. Therefore the behaviour
    of the (smaller mass) core is relatively unaffected by HD cooling.@eng
  bibo_authorlist:
  - foaf_Person:
      foaf_givenName: Greg L.
      foaf_name: Bryan, Greg L.
      foaf_surname: Bryan
  - foaf_Person:
      foaf_givenName: Ian D.
      foaf_name: McGreer, Ian D.
      foaf_surname: McGreer
  - foaf_Person:
      foaf_givenName: Andrei
      foaf_name: Mesinger, Andrei
      foaf_surname: Mesinger
  - foaf_Person:
      foaf_givenName: Zoltán
      foaf_name: Haiman, Zoltán
      foaf_surname: Haiman
      foaf_workInfoHomepage: http://www.librecat.org/personId=7c006e8c-cc0d-11ee-8322-cb904ef76f36
  bibo_doi: 10.1063/1.2905582
  dct_date: 2008^xs_gYear
  dct_isPartOf:
  - http://id.crossref.org/issn/0094-243X
  dct_language: eng
  dct_publisher: American Institute of Physics@
  dct_title: Feedback effects on population III star formation@
...