| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16c.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 8JMKD3MGP8W/35GGQPB |
| Repository | sid.inpe.br/mtc-m18@80/2009/06.19.18.06 (restricted access) |
| Last Update | 2009:12.08.11.33.12 (UTC) administrator |
| Metadata Repository | sid.inpe.br/mtc-m18@80/2009/06.19.18.06.03 |
| Metadata Last Update | 2020:04.28.17.48.41 (UTC) administrator |
| Secondary Key | INPE--PRE/ |
| DOI | 10.1088/0004-6256/137/1/296 |
| ISSN | 0004-6256 |
| Citation Key | DiazCies:2009:MuDoIm |
| Title | Multiline doppler imaging of MR SER in high state  |
| Year | 2009 |
| Month | Jan. |
| Access Date | 2024, Apr. 28 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 740 KiB |
| 2. Context | |
| Author | 1 Diaz, M. P. 2 Cieslinski, Deonísio |
| Group | 1 2 DAS-CEA-INPE-MCT-BR |
| Affiliation | 1 2 Instituto Nacional de Pesquisas Espaciais (INPE) |
| Author e-Mail Address | 1 marcos@astro.iag.usp.br 2 deo@das.inpe.br |
| Journal | Astronomical Journal |
| Volume | 137 |
| Number | 1 |
| Pages | 296-303 |
| History (UTC) | 2010-03-11 17:03:30 :: simone -> administrator :: 2010-05-11 01:08:21 :: administrator -> simone :: 2011-05-11 21:58:05 :: simone -> administrator :: 2020-04-28 17:48:41 :: administrator -> simone :: 2009 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Keywords | accretion accretion disks binaries: close line: formation novae cataclysmic variables X-rays: binaries |
| Abstract | Doppler images in Balmer, He I, He II and C II lines, and simultaneous I-band photometry of the polar MR Ser are presented and analyzed. The Balmer and Helium Doppler tomograms, of this bright polar at high mass transfer state show the emission from the accretion flow and the heated surface of the companion star. As a result of a comparison between the Doppler tomograms, the ionization structure of the flow could be constrained. The highest ionization region was found in the vicinity of the magnetospheric radius. Photoionization modeling of the accretion column indicates that the Balmer and Helium emission line production in this system can be explained only by the central soft X-ray illumination. The orbital ephemeris of MR Ser has been revised. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Multiline doppler imaging... |
| 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 | Diaz_Multiline.pdf |
| User Group | administrator simone |
| Visibility | shown |
| Archiving Policy | denypublisher denyfinaldraft |
| Read Permission | deny from all and allow from 150.163 |
| 5. Allied materials | |
| Mirror Repository | sid.inpe.br/mtc-m18@80/2008/03.17.15.17.24 |
| Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
| Dissemination | WEBSCI; PORTALCAPES. |
| Host Collection | sid.inpe.br/mtc-m18@80/2008/03.17.15.17 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage e-mailaddress format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
| 7. Description control | |
| e-Mail (login) | simone |
| update | |