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La astronomía nos enseña que el universo entero baila una especie de vals: miles de millones de satélites giran alrededor de planetas, que giran alrededor de estrellas, que giran alrededor de agujeros negros. A continuación, entérate de las últimas novedades de Sagitario A, nuestro agujero negro.


Ananna, TonimaTreister, EzequielUrry, C. MeganRicci, ClaudioHickox, R. C.Padmanabhan, NikhilMarchesi, StefanoKirkpatrick, Allison[Accretion History of AGNs. II. Constraints on AGN Spectral Parameters Using the Cosmic X-Ray Background, Accretion History of AGNs. II. Constraints on AGN Spectral Parameters Using the Cosmic X-Ray Background]Accretion History of AGNs. II. Constraints on AGN Spectral Parameters Using the Cosmic X-Ray Background

Zavala, Jorge A.Casey, Caitlin M.Scoville, Nick Z.Champagne, Jaclyn B.Chiang, Y.Dannerbauer, H.Drew, P.Fu, HaiSpilker, J.Treister, Ezequiel[On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z ≈ 2.0─2.5, On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z ≈ 2.0─2.5]On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z ≈ 2.0─2.5

Casey, Caitlin M.Zavala, Jorge A.Aravena, ManuelBethermin, M.Caputi, Karina I.Champagne, Jaclyn B.Clements, David L.Cunha, Elisabete daDrew, PatrickTreister, Ezequiel[Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85, Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85]Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at z = 5.85

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