Athari ya Sunyaev-Zel'dovich
Athari ya Sunyaev-Zel'dovich ni jambo ambapo msingi wa mawimbi ya sumakuumeme ya anga (CMB) hupotoshwa wakati fotoni zinapopitia gesi moto katika makundi ya galaksi. Athari hii, iliyopendekezwa na Rashid Sunyaev na Yakov Zel'dovich mwaka 1972, inatoa njia yenye nguvu ya kugundua makundi ya galaksi yaliyo mbali na kupima vigezo vya msingi vya ulimwengu bila dhana za umbali.
Soma mbinu kamili
Ingia kwa akaunti ya bure ili kusoma sehemu hii.
Ramani ya mbinu
Jirani ya mbinu zinazohusiana — chagua nodi ili kuchunguza.
Vyanzo
- Sunyaev, R. A., & Zel'dovich, Y. B. (1972). The observations of the relic radiation as a test of the nature of X-ray radiation from clusters of galaxies. Comments on Astrophysics and Space Physics, 4(4), 173-178. link ↗
- Carlstrom, J. E., Holder, G. P., & Reese, E. D. (2002). Cosmology with the Sunyaev-Zel'dovich effect. Annual Review of Astronomy and Astrophysics, 40, 643-680. DOI: 10.1146/annurev.astro.40.060401.093803 ↗
- Planck Collaboration (2014). Planck 2013 results. XXVII. Doppler boosting of the Sunyaev-Zel'dovich effect. Astronomy & Astrophysics, 571, A27. link ↗
Jinsi ya kunukuu ukurasa huu
ScholarGate. (2026, June 3). Sunyaev-Zel'dovich Effect for Galaxy Cluster Detection. ScholarGate. https://scholargate.app/sw/astronomy/sunyaev-zeldovich-effect
Mbinu ipi?
Weka mbinu hii kando ya jamaa zake wa karibu na uzisome bega kwa bega — maktaba huweka vitabu mezani; uamuzi ni wako.
- Mawimbi ya Sauti ya BaryonAstronomia↔ linganisha
- Uchambuzi wa Anisotropia ya CMBAstronomia↔ linganisha
- Unyevu Mkuu wa MnatoAstronomia↔ linganisha
Imerejelewa na
Similar methods
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