Temperature maps of X-ray emitting gas in simulated galaxy cluster mergers: the bullet-shaped morphology of Abell 3376 (2012)
- Authors:
- Autor USP: LIMA NETO, GASTAO CESAR BIERRENBACH - IAG
- Unidade: IAG
- Subjects: AGLOMERADOS DE GALÁXIAS; RAIOS X; GÁS INTERESTELAR; TEMPERATURA
- Language: Inglês
- Imprenta:
- Publisher: Sociedade Astronômica Brasileira
- Publisher place: São Paulo
- Date published: 2012
- Conference titles: Reunião Anual da Sociedade Astronômica Brasileira
-
ABNT
MACHADO, Rubens E. G e LIMA NETO, Gastão César Bierrenbach. Temperature maps of X-ray emitting gas in simulated galaxy cluster mergers: the bullet-shaped morphology of Abell 3376. 2012, Anais.. São Paulo: Sociedade Astronômica Brasileira, 2012. . Acesso em: 09 maio 2026. -
APA
Machado, R. E. G., & Lima Neto, G. C. B. (2012). Temperature maps of X-ray emitting gas in simulated galaxy cluster mergers: the bullet-shaped morphology of Abell 3376. In . São Paulo: Sociedade Astronômica Brasileira. -
NLM
Machado REG, Lima Neto GCB. Temperature maps of X-ray emitting gas in simulated galaxy cluster mergers: the bullet-shaped morphology of Abell 3376. 2012 ;[citado 2026 maio 09 ] -
Vancouver
Machado REG, Lima Neto GCB. Temperature maps of X-ray emitting gas in simulated galaxy cluster mergers: the bullet-shaped morphology of Abell 3376. 2012 ;[citado 2026 maio 09 ] - Relaxed and unrelaxed clusters of galaxies seen in X-rays
- The merging cluster of galaxies Abell 3376: an optical view
- Spiral-like structure at the centre of nearby clusters of galaxies
- The merging cluster Abell 85 caught between meals by XMM-Newton
- A comprehensive picture of baryons in groups and clusters of galaxies
- An XMM-Newton view of the cluster of galaxies Abell 85
- Galaxy cluster as probes for cosmology and dark matter
- Perfil de temperatura e fração de bárions de aglomerados de galáxias em diferentes REDSHIFTS
- Physical properties of abell 85 intra-cluster medium
- Stellar formation in Brightest Cluster Galaxies
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