| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZGivnJVY/M2hb6 |
| Repository | sid.inpe.br/mtc-m16@80/2006/08.01.19.03 (restricted access) |
| Last Update | 2006:08.01.19.03.33 (UTC) administrator |
| Metadata Repository | sid.inpe.br/mtc-m16@80/2006/08.01.19.03.35 |
| Metadata Last Update | 2018:06.05.01.16.54 (UTC) administrator |
| Secondary Key | INPE-13924--PRE/9104 |
| ISSN | 1742-6588 |
| Citation Key | AraújoMiraAgui:2006:ExNeSt |
| Title | Excitation of Neutron Star f-mode in Low Mass X-ray Binaries  |
| Year | 2006 |
| Access Date | 2024, May 16 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 97 KiB |
| 2. Context | |
| Author | 1 Araújo, José Carlos Neves de 2 Miranda, Oswaldo Duarte 3 Aguiar, Odylio Denys |
| Resume Identifier | 1 8JMKD3MGP5W/3C9JHGK 2 8JMKD3MGP5W/3C9JJ2G |
| Group | 1 DAS-INPE-MCT-BR 2 DAS-INPE-MCT-BR 3 DAS-INPE-MCT-BR |
| Affiliation | 1 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS) 2 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS) 3 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS) |
| Journal | Journal of Physics: Conference Series |
| Volume | 32 |
| Pages | 1-5 |
| History (UTC) | 2006-08-01 19:03:35 :: simone -> administrator :: 2012-07-17 12:47:33 :: administrator -> banon :: 2006 2012-09-27 18:28:27 :: banon -> administrator :: 2006 2018-06-05 01:16:54 :: administrator -> marciana :: 2006 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Abstract | Neutron Stars (NSs) present a host of pulsation modes. Only a few of them, however, is of relevance from the gravitational wave (GW) point of view. Among the various possible modes the pulsation energy is mostly stored in the f-mode in which the fluid parameters undergo the largest changes. An important question is how the pulsation modes are excited in NSs. Here we consider the excitation of the f-mode in the accreting NSs belonging to Low Mass X-ray Binaries (LMXBs), which may well be a recurrent source of GWs, since the NSs are continuously receiving matter from their companion stars. We also discuss the detectability of the GWs for the scenario considered here. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Excitation of Neutron... |
| doc Directory Content | access |
| source Directory Content | there are no files |
| agreement Directory Content | there are no files |
| 4. Conditions of access and use | |
| Language | en |
| Target File | Excitation of neutron star f mode in low.pdf |
| User Group | administrator banon simone |
| Visibility | shown |
| Copy Holder | SID/SCD |
| Archiving Policy | denypublisher denyfinaldraft12 |
| Read Permission | deny from all and allow from 150.163 |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
| Dissemination | WEBSCI; PORTALCAPES; COMPENDEX. |
| Host Collection | sid.inpe.br/banon/2003/08.15.17.40 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn keywords label lineage mark mirrorrepository month nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
| 7. Description control | |
| e-Mail (login) | marciana |
| update | |