Aviso: para depositar documentos, por favor, inicia sesión e identifícate con tu cuenta de correo institucional de la UCM con el botón MI CUENTA UCM. No emplees la opción AUTENTICACIÓN CON CONTRASEÑA
 

Distribution of baryonic and non-baryonic matter in clusters of galaxies

dc.book.titleTracing cosmic evolution with galaxy clusters, proceedings
dc.contributor.authorCastillo Morales, María África
dc.contributor.authorSchindler, S.
dc.date.accessioned2023-06-20T21:11:28Z
dc.date.available2023-06-20T21:11:28Z
dc.date.issued2002
dc.descriptionWorkshop on Tracing Cosmic Evolution with Galaxy Clusters (2001. Sesto Pusteria, Italy). We would like to thank the organizers of the meeting for the financial support. We thank Javier Campania for the help printing the poster.
dc.description.abstractWe present the analysis of baryonic and non-baryonic matter distributions in a sample of eleven nearby clusters (0.03 < z < 0.09) with temperatures between 4.4 and 9.4 keV. These galaxy clusters have been studied in detail using X-ray data and global physical properties have been determined. Correlations between these quantities have been analysed and compared with the results for distant clusters. We found an interesting dependence between the relative gas extent (expressed as the ratio of gas mass fractions at r(500) and 0.5 x r(500)) and the total cluster mass. The extent of the gas relative to the extent of the dark matter tends to be larger in less massive clusters. This dependence might give us some hints about non-gravitational processes in clusters.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/30621
dc.identifier.isbn1-58381-108-7
dc.identifier.officialurlhttp://arxiv.org/pdf/astro-ph/0106201v1.pdf
dc.identifier.urihttps://hdl.handle.net/20.500.14352/60926
dc.issue.number268
dc.language.isoeng
dc.page.final352
dc.page.initial351
dc.publisherAstronomical Soc. Pacific
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordAstronomy and astrophysics
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.titleDistribution of baryonic and non-baryonic matter in clusters of galaxies
dc.typebook part
dc.volume.number268
dcterms.references1. Fukazawa, Y. 1997, Ph.D. thesis, Univ. Tokyo. 2. Allen S.W. & Fabian A.C., Mon. Not. R. Astr. Soc. 297, 57 (1998). 3. Arnaud M. & Evrard A.E., Mon. Not. R. Astr. Soc. 305, 631 (1999). 4. Ettori S. & Fabian A.C., Mon. Not. R. Astr. Soc. 305, 834 (1999). 5. Horner D.J., et al, Astrophys. J. 520, 78 (1999). 6. Jones C. & Forman W.R., Astrophys. J. 511, 65 (1999). 7. Mohr J.J., et al, Astrophys. J. 517, 627 (1999). 8. Schindler S., Astron. Astrophys. 349, 435 (1999). 9. Schindler S., et al, Astron. Astrophys submitted (2001). 10. Neumann D.M.& Arnaud M., Astron. Astrophys. 348, 711 (1999). 11. Stanford S.A., et al, Astrophysical Journal in press, astro-ph/0012250. 12. Cavaliere A. & Fusco-Fermiano F., Astron. Astrophys. 49, 137 (1976). 13. Peres C.B., et al, Mon. Not. R. Astr. Soc. 298, 416 (1998). 14. Allen S.W. & Fabian A.C., Mon. Not. R. Astr. Soc. 286, 583 (1997). 15. White D.A, et al, Mon. Not. R. Astr. Soc. 292, 419 (1997). 16. Markevitch M., et al, Astrophys. J. 503, 77 (1998). 17. White D.A, Mon. Not. R. Astr. Soc. 312, 663 (2000). 18. Irwin, J.A & Bregman, J.N., Astrophys. J. 538, 543 (2000). 19. Evrard A., et al, Astrophys. J. 469, 494 (1996). 20. Matsumoto H., et al, Publ. Astr. Soc. Japan. 52, 153 (2000). 21. Reiprich T.H. & Böhringer H., Proceedings of the Workshop ‘Diffuse thermal and relativistic plasma in galaxy cluster’. Ringberg Castle, Germany, April 19-23, 1999, p.157.
dspace.entity.typePublication
relation.isAuthorOfPublication2f955c06-40a8-47c2-89f2-bd5458272bad
relation.isAuthorOfPublication.latestForDiscovery2f955c06-40a8-47c2-89f2-bd5458272bad

Download

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
castillo19preprint.pdf
Size:
149.98 KB
Format:
Adobe Portable Document Format