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1. Identity statement Reference Type Book Section Site mtc-m21c.sid.inpe.br Holder Code isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S Identifier 8JMKD3MGP3W34R/3UTKC8P Repository sid.inpe.br/mtc-m21c/2020/02.10.17.23   (restricted access) Last Update 2020:02.10.17.23.38 (UTC) simone Metadata Repository sid.inpe.br/mtc-m21c/2020/02.10.17.23.38 Metadata Last Update 2022:03.15.18.56.38 (UTC) administrator Secondary Key INPE--PRE/ ISBN 978-3-030-16077-7 Citation Key PereiraSantCamp:2019:ToSuBl Title Towards the super-massive black hole seeds Year 2019 Access Date 2025, Apr. 26 Secondary Type PRE LI Number of Files 1 Size 345 KiB 2. Context Author 1 Pereira, Eduardo dos Santos 2 Santos, Pedro Alexandre dos 3 Campos Velho, Haroldo Fraga de Resume Identifier 1 2 3 8JMKD3MGP5W/3C9JHC3 Group 1 COCST-COCST-INPE-MCTIC-GOV-BR 2 LABAC-COCTE-INPE-MCTIC-GOV-BR 3 LABAC-COCTE-INPE-MCTIC-GOV-BR Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 Instituto Nacional de Pesquisas Espaciais (INPE) Author e-Mail Address 1 eduardo.santos@inpe.br 2 pedro.alexandre@inpe.br 3 haroldo.camposvelho@inpe.br Editor Constanda, Christian Harris, Paul Book Title Integral methods in science and engineering Publisher Springer City Brighton, UK Pages 333-342 History (UTC) 2020-02-10 17:23:38 :: simone -> administrator :: 2022-03-15 18:56:38 :: administrator -> simone :: 2019 3. Content and structure Is the master or a copy? is the master Content Stage completed Transferable 1 Content Type External Contribution Version Type publisher Keywords black holes Abstract In science, there are different problems to be solved. One of them is the evolution of the Universe. This paper discusses a little piece of the cited problem, which is the evolution of the black holes. From nowadays, observations show super-massive black holes with mass about 109M3 are ubiquitous in galaxy centers. However, the origin of this kind of object is not completely understood yet. A possibility rely in the fact the super-massive black holes (SMBH) seeds had their origin in the death of the Population III stars, during the called Dark Cosmological Ages at redshift in the interval z = [10, 20]. In order to verify this hypothesis, the first step is to try to reconstruct the SMBH mass function at high redshift. The next step is to do a comparison between the computed distribution with the reminiscent of the first stars. Area COMP Arrangement 1 urlib.net > BDMCI > Fonds > Produção anterior à 2021 > LABAC > Towards the super-massive... Arrangement 2 urlib.net > BDMCI > Fonds > Produção anterior à 2021 > COCST > Towards the super-massive... doc Directory Content access source Directory Content there are no files agreement Directory Content agreement.html 10/02/2020 14:23 1.8 KiB  4. Conditions of access and use Language en Target File pereira_towards.pdf User Group simone Visibility shown Read Permission deny from all and allow from 150.163 Update Permission not transferred 5. Allied materials Next Higher Units 8JMKD3MGPCW/3ESGTTP 8JMKD3MGPCW/3F3T29H Host Collection urlib.net/www/2017/11.22.19.04 6. Notes Empty Fields archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition format issn label lineage mark mirrorrepository nextedition notes numberofvolumes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark serieseditor seriestitle session shorttitle sponsor subject tertiarymark tertiarytype translator url volume 7. Description control e-Mail (login) simone update

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