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24 results on '"Borgani, S."'

1. The Spiderweb Protocluster is Being Magnetized by Its Central Radio Jet

Author

Anderson, Craig S., primary, Carilli, Christopher L., additional, Tozzi, Paolo, additional, Miley, G. K., additional, Borgani, S., additional, Clarke, Tracy, additional, Di Mascolo, Luca, additional, Liu, Ang, additional, Mroczkowski, Tony, additional, Pannella, Maurilio, additional, Pentericci, L., additional, Rottgering, H. J. A., additional, and Saro, A., additional

Published
2022
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2. X-Ray Emission from the Jets and Lobes of the Spiderweb

Author

Carilli, Christopher L., primary, Anderson, Craig S., additional, Tozzi, Paolo, additional, Pannella, Maurilio, additional, Clarke, Tracy, additional, Pentericci, L., additional, Liu, Ang, additional, Mroczkowski, Tony, additional, Miley, G. K., additional, Rottgering, H. J., additional, Borgani, S., additional, Norman, Colin, additional, Saro, A., additional, Nonino, M., additional, and Di Mascolo, L., additional

Published
2022
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3. The X-Ray Halo Scaling Relations of Supermassive Black Holes

Author

Gaspari, M., primary, Eckert, D., additional, Ettori, S., additional, Tozzi, P., additional, Bassini, L., additional, Rasia, E., additional, Brighenti, F., additional, Sun, M., additional, Borgani, S., additional, Johnson, S. D., additional, Tremblay, G. R., additional, Stone, J. M., additional, Temi, P., additional, Yang, H.-Y. K., additional, Tombesi, F., additional, and Cappi, M., additional

Published
2019
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6. COOL CORE CLUSTERS FROM COSMOLOGICAL SIMULATIONS

Author

Rasia, E., primary, Borgani, S., additional, Murante, G., additional, Planelles, S., additional, Beck, A. M., additional, Biffi, V., additional, Ragone-Figueroa, C., additional, Granato, G. L., additional, Steinborn, L. K., additional, and Dolag, K., additional

Published
2015
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7. CLASH-VLT: INSIGHTS ON THE MASS SUBSTRUCTURES IN THE FRONTIER FIELDS CLUSTER MACS J0416.1–2403 THROUGH ACCURATE STRONG LENS MODELING

Author

Grillo, C., primary, Suyu, S. H., additional, Rosati, P., additional, Mercurio, A., additional, Balestra, I., additional, Munari, E., additional, Nonino, M., additional, Caminha, G. B., additional, Lombardi, M., additional, De Lucia, G., additional, Borgani, S., additional, Gobat, R., additional, Biviano, A., additional, Girardi, M., additional, Umetsu, K., additional, Coe, D., additional, Koekemoer, A. M., additional, Postman, M., additional, Zitrin, A., additional, Halkola, A., additional, Broadhurst, T., additional, Sartoris, B., additional, Presotto, V., additional, Annunziatella, M., additional, Maier, C., additional, Fritz, A., additional, Vanzella, E., additional, and Frye, B., additional

Published
2015
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8. CHANDRADEEP OBSERVATION OF XDCP J0044.0-2033, A MASSIVE GALAXY CLUSTER ATz> 1.5

Author

Tozzi, P., primary, Santos, J. S., additional, Jee, M. J., additional, Fassbender, R., additional, Rosati, P., additional, Nastasi, A., additional, Forman, W., additional, Sartoris, B., additional, Borgani, S., additional, Boehringer, H., additional, Altieri, B., additional, Pratt, G. W., additional, Nonino, M., additional, and Jones, C., additional

Published
2015
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10. CHANDRAVIEW OF THE WARM-HOT INTERGALACTIC MEDIUM TOWARD 1ES 1553+113: ABSORPTION-LINE DETECTIONS AND IDENTIFICATIONS. I.

Author

Nicastro, F., primary, Elvis, M., additional, Krongold, Y., additional, Mathur, S., additional, Gupta, A., additional, Danforth, C., additional, Barcons, X., additional, Borgani, S., additional, Branchini, E., additional, Cen, R., additional, Davé, R., additional, Kaastra, J., additional, Paerels, F., additional, Piro, L., additional, Shull, J. M., additional, Takei, Y., additional, and Zappacosta, L., additional

Published
2013
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14. The Diffuse Light in Simulations of Galaxy Clusters

Author

Murante, G., primary, Arnaboldi, M., additional, Gerhard, O., additional, Borgani, S., additional, Cheng, L. M., additional, Diaferio, A., additional, Dolag, K., additional, Moscardini, L., additional, Tormen, G., additional, Tornatore, L., additional, and Tozzi, P., additional

Published
2004
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17. Tracing the Large‐Scale Structure in theChandraDeep Field South

Author

Gilli, R., primary, Cimatti, A., additional, Daddi, E., additional, Hasinger, G., additional, Rosati, P., additional, Szokoly, G., additional, Tozzi, P., additional, Bergeron, J., additional, Borgani, S., additional, Giacconi, R., additional, Kewley, L., additional, Mainieri, V., additional, Mignoli, M., additional, Nonino, M., additional, Norman, C., additional, Wang, J., additional, Zamorani, G., additional, Zheng, W., additional, and Zirm, A., additional

Published
2003
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18. The Chandra Deep Field–South: The 1 Million Second Exposure

Author

Rosati, P., primary, Tozzi, P., additional, Giacconi, R., additional, Gilli, R., additional, Hasinger, G., additional, Kewley, L., additional, Mainieri, V., additional, Nonino, M., additional, Norman, C., additional, Szokoly, G., additional, Wang, J. X., additional, Zirm, A., additional, Bergeron, J., additional, Borgani, S., additional, Gilmozzi, R., additional, Grogin, N., additional, Koekemoer, A., additional, Schreier, E., additional, and Zheng, W., additional

Published
2002
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19. New Results from the X‐Ray and Optical Survey of the Chandra Deep Field–South: The 300 Kilosecond Exposure. II.

Author

Tozzi, P., primary, Rosati, P., additional, Nonino, M., additional, Bergeron, J., additional, Borgani, S., additional, Gilli, R., additional, Gilmozzi, R., additional, Hasinger, G., additional, Grogin, N., additional, Kewley, L., additional, Koekemoer, A., additional, Norman, C., additional, Schreier, E., additional, Szokoly, G., additional, Wang, J. X., additional, Zheng, W., additional, Zirm, A., additional, and Giacconi, R., additional

Published
2001
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24. The X-Ray Halo Scaling Relations of Supermassive Black Holes

Author

Stefano Ettori, Massimo Gaspari, Sean D. Johnson, Fabrizio Brighenti, Francesco Tombesi, Dominique Eckert, Stefano Borgani, Pasquale Temi, Grant R. Tremblay, Paolo Tozzi, James M. Stone, Elena Rasia, L. Bassini, Massimo Cappi, Mouyuan Sun, H. Y. K. Yang, Gaspari M., Eckert D., Ettori S., Tozzi P., Bassini L., Rasia E., Brighenti F., Sun M., Borgani S., Johnson S.D., Tremblay G.R., Stone J.M., Temi P., Yang H.-Y.K., Tombesi F., Cappi M., Gaspari, M., Eckert, D., Ettori, S., Tozzi, P., Bassini, L., Rasia, E., Brighenti, F., Sun, M., Borgani, S., Johnson, S. D., Tremblay, G. R., Stone, J. M., Temi, P., Yang, H. -Y. K., Tombesi, F., and Cappi, M.

Subjects
Late-type galaxie, 010504 meteorology & atmospheric sciences, Optical observation, Elliptical galaxie, Hydrodynamical simulation, Astrophysics, 01 natural sciences, Lenticular galaxies, Interstellar medium, Supermassive black holes, Astrophysics - Cosmology and Nongalactic Astrophysic, 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Sigma, Brightest cluster galaxie, Elliptical galaxy, Halo, Astrophysics - High Energy Astrophysical Phenomena, Lenticular galaxie, Astrophysics - Cosmology and Nongalactic Astrophysics, Circumgalactic medium, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astrophysics::High Energy Astrophysical Phenomena, Hydrodynamical simulations, Dark matter, FOS: Physical sciences, Brightest cluster galaxies, Elliptical galaxies, Late-type galaxies, Intracluster medium, X-ray astronomy, Astrophysics - Astrophysics of Galaxies, Physics - Plasma Physics, Astrophysics::Cosmology and Extragalactic Astrophysics, Settore FIS/05 - Astronomia e Astrofisica, Astrophysics - Astrophysics of Galaxie, Supermassive black hole, 0103 physical sciences, Lenticular galaxy, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Astronomy and Astrophysics, Galaxy, Plasma Physics (physics.plasm-ph), Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA)
Abstract

We carry out a comprehensive Bayesian correlation analysis between hot halos and direct masses of supermassive black holes (SMBHs), by retrieving the X-ray plasma properties (temperature, luminosity, density, pressure, masses) over galactic to cluster scales for 85 diverse systems. We find new key scalings, with the tightest relation being the $M_\bullet-T_{\rm x}$, followed by $M_\bullet-L_{\rm x}$. The tighter scatter (down to 0.2 dex) and stronger correlation coefficient of all the X-ray halo scalings compared with the optical counterparts (as the $M_\bullet-\sigma_{\rm e}$) suggest that plasma halos play a more central role than stars in tracing and growing SMBHs (especially those that are ultramassive). Moreover, $M_\bullet$ correlates better with the gas mass than dark matter mass. We show the important role of the environment, morphology, and relic galaxies/coronae, as well as the main departures from virialization/self-similarity via the optical/X-ray fundamental planes. We test the three major channels for SMBH growth: hot/Bondi-like models have inconsistent anti-correlation with X-ray halos and too low feeding; cosmological simulations find SMBH mergers as sub-dominant over most of the cosmic time and too rare to induce a central-limit-theorem effect; the scalings are consistent with chaotic cold accretion (CCA), the rain of matter condensing out of the turbulent X-ray halos that sustains a long-term self-regulated feedback loop. The new correlations are major observational constraints for models of SMBH feeding/feedback in galaxies, groups, and clusters (e.g., to test cosmological hydrodynamical simulations), and enable the study of SMBHs not only through X-rays, but also via the Sunyaev-Zel'dovich effect (Compton parameter), lensing (total masses), and cosmology (gas fractions)., Comment: 40 pages, 27 figures, 3 tables; ApJ accepted version (minor revision) - Reviewer: "The authors are to be congratulated on a very interesting paper that deserves to be read by anyone interested in the connection between the SMBH and host galaxy."

Published
2019

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