دورية أكاديمية

The Variability of the Black Hole Image in M87 at the Dynamical Timescale

التفاصيل البيبلوغرافية
العنوان: The Variability of the Black Hole Image in M87 at the Dynamical Timescale
المؤلفون: Satapathy, Kaushik, Psaltis, Dimitrios, Ozel, Feryal, Medeiros, Lia, Dougall, Sean T., Chan, Chi-Kwan, Wielgus, Maciek, Prather, Ben S., Wong, George N., Gammie, Charles F., Akiyama, Kazunori, Alberdi, Antxon, Alef, Walter, Algaba, Juan Carlos, Anantua, Richard, Asada, Keiichi, Azulay, Rebecca, Baczko, Anne-Kathrin, Ball, David, Balokovic, Mislay, Barrett, John, Benson, Bradford A., Bintley, Dan, Blackburn, Lindy, Blundell, Raymond, Boland, Wilfred, Bouman, Katherine L., Bower, Geoffrey C., Boyce, Hope, Bremer, Michael, Brinkerink, Christiaan D., Brissenden, Roger, Britzen, Silke, Broderick, Avery E., Broguiere, Dominique, Bronzwaer, Thomas, Bustamente, Sandra, Byun, Do-Young, Carlstrom, John E., Chael, Andrew, Chatterjee, Koushik, Chatterjee, Shami, Chen, Ming-Tang, Chen, Yongjun, Cho, Ilje, Christian, Pierre, Conway, John E., Cordes, James M., Crawford, Thomas M., Crew, Geoffrey B., Cruz-Osorio, Alejandro, Cui, Yuzhu, Davelaar, Jordy, De Laurentis, Mariafelicia, Deane, Roger, Dempsey, Jessica, Desvignes, Gregory, Dexter, Jason, Doeleman, Sheperd S., Eatough, Ralph P., Falcke, Heino, Farah, Joseph, Fish, Vincent L., Fomalont, Ed, Ford, H. Alyson, Fraga-Encinas, Raquel, Friberg, Per, Fromm, Christian M., Fuentes, Antonio, Galison, Peter, Garcia, Roberto, Gentaz, Olivier, Georgiev, Boris, Goddi, Ciriaco, Gold, Roman, Gomez-Ruiz, Arturo, Gomez, Jose L., Gu, Minfeng, Gurwell, Mark, Hada, Kazuhiro, Haggard, Daryl, Hecht, Michael H., Hesper, Ronald, Ho, Paul, Honma, Mareki, Huang, Chih-Wei L., Huang, Lei, Hughes, David H., Ikeda, Shiro, Inoue, Makoto, Issaoun, Sara, James, David J., Jannuzi, Buell T., Janssen, Michael, Jeter, Britton, Jiang, Wu, Jimenez-Rosales, Alejandra, Johnson, Michael D., Jorstad, Svetlana, Jung, Taehyun, Karami, Mansour, Karuppusamy, Ramesh, Kawashima, Tomohisa, Keating, Garrett K., Kettenis, Mark, Kim, Dong-Jin, Kim, Jae-Young, Kim, Jongsoo, Kim, Junhan, Kino, Motoki, Koay, Jun Yi, Kofuji, Yutaro, Koch, Patrick M., Koyama, Shoko, Kramer, Carsten, Kramer, Michael, Krichbaum, Thomas P., Kuo, Cheng-Yu, Lauer, Tod R., Lee, Sang-Sung, Levis, Aviad, Li, Yan-Rong, Li, Zhiyuan, Lindqvist, Michael, Lico, Rocco, Lindahl, Greg, Liu, Jun, Liu, Kuo, Liuzzo, Elisabetta, Lo, Wen-Ping, Lobanov, Andrei P., Loinard, Laurent, Lonsdale, Colin, Lu, Ru-Sen, MacDonald, Nicholas R., Mao, Jirong, Marchili, Nicola, Markoff, Sera, Marrone, Daniel P., Marscher, Alan P., Marti-Vidal, Ivan, Matsushita, Satoki, Matthews, Lynn D., Menten, Karl M., Mizuno, Izumi, Mizuno, Yosuke, Moran, James M., Moriyama, Kotaro, Moscibrodzka, Monika, Mueller, Cornelia, Mejias, Alejandro Mus, Musoke, Gibwa, Nagai, Hiroshi, Nagar, Neil M., Nakamura, Masanori, Narayan, Ramesh, Narayanan, Gopal, Natarajan, Iniyan, Nathanail, Antonios, Neilsen, Joey, Neri, Roberto, Ni, Chunchong, Noutsos, Aristeidis, Nowak, Michael A., Okino, Hiroki, Olivares, Hector, Ortiz-Leon, Gisela N., Oyama, Tomoaki, Palumbo, Daniel C. M., Park, Jongho, Patel, Nimesh, Pen, Ue-Li, Pesce, Dominic W., Pietu, Vincent, Plambeck, Richard, PopStefanija, Aleksandar, Porth, Oliver, Potzl, Felix M., Preciado-Lopez, Jorge A., Pu, Hung-Yi, Ramakrishnan, Venkatessh, Rao, Ramprasad, Rawlings, Mark G., Raymond, Alexander W., Rezzolla, Luciano, Ripperda, Bart, Roelofs, Freek, Rogers, Alan, Ros, Eduardo, Rose, Mel, Roshanineshat, Arash, Rottmann, Helge, Roy, Alan L., Ruszczyk, Chet, Rygl, Kazi L. J., Sanchez, Salvador, Sanchez-Arguelles, David, Sasada, Mahito, Savolainen, Tuomas, Schloerb, F. Peter, Schuster, Karl-Friedrich, Shao, Lijing, Shen, Zhiqiang, Small, Des, Sohn, Bong Won, SooHoo, Jason, Sun, He, Tazaki, Fumie, Tetarenko, Alexandra J., Tiede, Paul, Tilanus, Remo P. J., Titus, Michael, Toma, Kenji, Torne, Pablo, Traianou, Efthalia, Trent, Tyler, Trippe, Sascha, van Bemmel, Ilse, van Langevelde, Huib Jan, van Rossum, Daniel R., Wagner, Jan, Ward-Thompson, Derek, Wardle, John, Weintroub, Jonathan, Wex, Norbert, Wharton, Robert, Wiik, Kaj, Wu, Qingwen, Yoon, Doosoo, Young, Andre, Young, Ken, Younsi, Ziri, Yuan, Feng, Yuan, Ye-Fei, Zensus, J. Anton, Zhao, Guang-Yao, Zhao, Shan-Shan
المساهمون: Department of Electronics and Nanoengineering, Metsähovi Radio Observatory, Anne Lähteenmäki Group, Aalto-yliopisto, Aalto University
بيانات النشر: IOP Publishing Ltd.
سنة النشر: 2022
المجموعة: Aalto University Publication Archive (Aaltodoc) / Aalto-yliopiston julkaisuarkistoa
مصطلحات موضوعية: GRMHD SIMULATIONS, ACCRETION, SCHEME, ENERGY, NOISE, MASS
الوصف: openaire: EC/H2020/610058/EU//BLACKHOLECAM | openaire: EC/H2020/730562/EU//RadioNet ; The black hole images obtained with the Event Horizon Telescope (EHT) are expected to be variable at the dynamical timescale near their horizons. For the black hole at the center of the M87 galaxy, this timescale (5-61 days) is comparable to the 6 day extent of the 2017 EHT observations. Closure phases along baseline triangles are robust interferometric observables that are sensitive to the expected structural changes of the images but are free of station-based atmospheric and instrumental errors. We explored the day-to-day variability in closure-phase measurements on all six linearly independent nontrivial baseline triangles that can be formed from the 2017 observations. We showed that three triangles exhibit very low day-to-day variability, with a dispersion of ∼3°-5°. The only triangles that exhibit substantially higher variability (∼90°-180°) are the ones with baselines that cross the visibility amplitude minima on the u-v plane, as expected from theoretical modeling. We used two sets of general relativistic magnetohydrodynamic simulations to explore the dependence of the predicted variability on various black hole and accretion-flow parameters. We found that changing the magnetic field configuration, electron temperature model, or black hole spin has a marginal effect on the model consistency with the observed level of variability. On the other hand, the most discriminating image characteristic of models is the fractional width of the bright ring of emission. Models that best reproduce the observed small level of variability are characterized by thin ring-like images with structures dominated by gravitational lensing effects and thus least affected by turbulence in the accreting plasmas. ; Peer reviewed
نوع الوثيقة: article in journal/newspaper
وصف الملف: application/pdf
اللغة: English
تدمد: 0004-637X
العلاقة: info:eu-repo/grantAgreement/EC/H2020/730562/EU//RadioNet; Astrophysical Journal; Volume 925, issue 1; Satapathy, K, Psaltis, D, Ozel, F, Medeiros, L, Dougall, S T, Chan, C-K, Wielgus, M, Prather, B S, Wong, G N, Gammie, C F, Akiyama, K, Alberdi, A, Alef, W, Algaba, J C, Anantua, R, Asada, K, Azulay, R, Baczko, A-K, Ball, D, Balokovic, M, Barrett, J, Benson, B A, Bintley, D, Blackburn, L, Blundell, R, Boland, W, Bouman, K L, Bower, G C, Boyce, H, Bremer, M, Brinkerink, C D, Brissenden, R, Britzen, S, Broderick, A E, Broguiere, D, Bronzwaer, T, Bustamente, S, Byun, D-Y, Carlstrom, J E, Chael, A, Chatterjee, K, Chatterjee, S, Chen, M-T, Chen, Y, Cho, I, Christian, P, Conway, J E, Cordes, J M, Crawford, T M, Crew, G B, Cruz-Osorio, A, Cui, Y, Davelaar, J, De Laurentis, M, Deane, R, Dempsey, J, Desvignes, G, Dexter, J, Doeleman, S S, Eatough, R P, Falcke, H, Farah, J, Fish, V L, Fomalont, E, Ford, H A, Fraga-Encinas, R, Friberg, P, Fromm, C M, Fuentes, A, Galison, P, Garcia, R, Gentaz, O, Georgiev, B, Goddi, C, Gold, R, Gomez-Ruiz, A, Gomez, J L, Gu, M, Gurwell, M, Hada, K, Haggard, D, Hecht, M H, Hesper, R, Ho, P, Honma, M, Huang, C-W L, Huang, L, Hughes, D H, Ikeda, S, Inoue, M, Issaoun, S, James, D J, Jannuzi, B T, Janssen, M, Jeter, B, Jiang, W, Jimenez-Rosales, A, Johnson, M D, Jorstad, S, Jung, T, Karami, M, Karuppusamy, R, Kawashima, T, Keating, G K, Kettenis, M, Kim, D-J, Kim, J-Y, Kim, J, Kim, J, Kino, M, Koay, J Y, Kofuji, Y, Koch, P M, Koyama, S, Kramer, C, Kramer, M, Krichbaum, T P, Kuo, C-Y, Lauer, T R, Lee, S-S, Levis, A, Li, Y-R, Li, Z, Lindqvist, M, Lico, R, Lindahl, G, Liu, J, Liu, K, Liuzzo, E, Lo, W-P, Lobanov, A P, Loinard, L, Lonsdale, C, Lu, R-S, MacDonald, N R, Mao, J, Marchili, N, Markoff, S, Marrone, D P, Marscher, A P, Marti-Vidal, I, Matsushita, S, Matthews, L D, Menten, K M, Mizuno, I, Mizuno, Y, Moran, J M, Moriyama, K, Moscibrodzka, M, Mueller, C, Mejias, A M, Musoke, G, Nagai, H, Nagar, N M, Nakamura, M, Narayan, R, Narayanan, G, Natarajan, I, Nathanail, A, Neilsen, J, Neri, R, Ni, C, Noutsos, A, Nowak, M A, Okino, H, Olivares, H, Ortiz-Leon, G N, Oyama, T, Palumbo, D C M, Park, J, Patel, N, Pen, U-L, Pesce, D W, Pietu, V, Plambeck, R, PopStefanija, A, Porth, O, Potzl, F M, Preciado-Lopez, J A, Pu, H-Y, Ramakrishnan, V, Rao, R, Rawlings, M G, Raymond, A W, Rezzolla, L, Ripperda, B, Roelofs, F, Rogers, A, Ros, E, Rose, M, Roshanineshat, A, Rottmann, H, Roy, A L, Ruszczyk, C, Rygl, K L J, Sanchez, S, Sanchez-Arguelles, D, Sasada, M, Savolainen, T, Schloerb, F P, Schuster, K-F, Shao, L, Shen, Z, Small, D, Sohn, B W, SooHoo, J, Sun, H, Tazaki, F, Tetarenko, A J, Tiede, P, Tilanus, R P J, Titus, M, Toma, K, Torne, P, Traianou, E, Trent, T, Trippe, S, van Bemmel, I, van Langevelde, H J, van Rossum, D R, Wagner, J, Ward-Thompson, D, Wardle, J, Weintroub, J, Wex, N, Wharton, R, Wiik, K, Wu, Q, Yoon, D, Young, A, Young, K, Younsi, Z, Yuan, F, Yuan, Y-F, Zensus, J A, Zhao, G-Y & Zhao, S-S 2022, ' The Variability of the Black Hole Image in M87 at the Dynamical Timescale ', The Astrophysical Journal, vol. 925, no. 1, 13 . https://doi.org/10.3847/1538-4357/ac332eTest; PURE UUID: 2f7c9691-7b40-4fd5-89e1-ef2a875d05b2; PURE ITEMURL: https://research.aalto.fi/en/publications/2f7c9691-7b40-4fd5-89e1-ef2a875d05b2Test; PURE LINK: http://www.scopus.com/inward/record.url?scp=85125877065&partnerID=8YFLogxKTest; PURE FILEURL: https://research.aalto.fi/files/79571453/The_Variability_of_the_Black_Hole_Image_in_M87_at_the_Dynamical_Timescale.pdfTest; https://aaltodoc.aalto.fi/handle/123456789/113098Test; URN:NBN:fi:aalto-202202231986
DOI: 10.3847/1538-4357/ac332e
الإتاحة: https://doi.org/10.3847/1538-4357/ac332eTest
https://aaltodoc.aalto.fi/handle/123456789/113098Test
حقوق: openAccess
رقم الانضمام: edsbas.8A63E5AB
قاعدة البيانات: BASE
الوصف
تدمد:0004637X
DOI:10.3847/1538-4357/ac332e