Chasing the Break: Tracing the Full Evolution of a Black Hole X-Ray Binary Jet with Multiwavelength Spectral Modeling
Black hole (BH) X-ray binaries (XRBs) are ideal targets to study the connection between accretion inflow and jet outflow. Here we present quasi-simultaneous, multiwavelength observations of the Galactic BH system MAXI J1820+070, throughout its 2018–2019 outburst. Our data set includes coverage from...
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IOP Publishing
2024-01-01
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Online Access: | https://doi.org/10.3847/1538-4357/ad1a10 |
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author | Constanza Echiburú-Trujillo Alexandra J. Tetarenko Daryl Haggard Thomas D. Russell Karri I. I. Koljonen Arash Bahramian Jingyi Wang Michael Bremer Joe Bright Piergiorgio Casella David M. Russell Diego Altamirano M. Cristina Baglio Tomaso Belloni Chiara Ceccobello Stephane Corbel Maria Diaz Trigo Dipankar Maitra Aldrin Gabuya Elena Gallo Sebastian Heinz Jeroen Homan Erin Kara Elmar Körding Fraser Lewis Matteo Lucchini Sera Markoff Simone Migliari James C. A. Miller-Jones Jerome Rodriguez Payaswini Saikia Craig L. Sarazin Tariq Shahbaz Gregory Sivakoff Roberto Soria Vincenzo Testa Bailey E. Tetarenko Valeriu Tudose |
author_facet | Constanza Echiburú-Trujillo Alexandra J. Tetarenko Daryl Haggard Thomas D. Russell Karri I. I. Koljonen Arash Bahramian Jingyi Wang Michael Bremer Joe Bright Piergiorgio Casella David M. Russell Diego Altamirano M. Cristina Baglio Tomaso Belloni Chiara Ceccobello Stephane Corbel Maria Diaz Trigo Dipankar Maitra Aldrin Gabuya Elena Gallo Sebastian Heinz Jeroen Homan Erin Kara Elmar Körding Fraser Lewis Matteo Lucchini Sera Markoff Simone Migliari James C. A. Miller-Jones Jerome Rodriguez Payaswini Saikia Craig L. Sarazin Tariq Shahbaz Gregory Sivakoff Roberto Soria Vincenzo Testa Bailey E. Tetarenko Valeriu Tudose |
author_sort | Constanza Echiburú-Trujillo |
collection | DOAJ |
description | Black hole (BH) X-ray binaries (XRBs) are ideal targets to study the connection between accretion inflow and jet outflow. Here we present quasi-simultaneous, multiwavelength observations of the Galactic BH system MAXI J1820+070, throughout its 2018–2019 outburst. Our data set includes coverage from the radio through X-ray bands from 17 different instruments/telescopes, and encompasses 19 epochs over a 7 month period, resulting in one of the most well-sampled multiwavelength data sets of a BH XRB outburst to date. With our data, we compile and model the broadband spectra of this source using a phenomenological model that includes emission from the jet, a companion star, and an accretion flow. This modeling allows us to track the evolution of the spectral break in the jet spectrum, a key observable that samples the jet launching region. We find that the spectral break location changes over at least ≈3 orders of magnitude in electromagnetic frequency over this period. Using these spectral break measurements, we link the full cycle of jet behavior, including the rising, quenching, and reignition, to the changing accretion flow properties as the source evolves through its different accretion states. Our analysis shows consistent jet behavior with other sources in similar phases of their outbursts, reinforcing the idea that jet quenching and recovery may be a global feature of BH XRB systems in outburst. Our results also provide valuable evidence supporting a close connection between the geometry of the inner accretion flow and the base of the jet. |
first_indexed | 2024-03-08T02:52:58Z |
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institution | Directory Open Access Journal |
issn | 1538-4357 |
language | English |
last_indexed | 2024-03-08T02:52:58Z |
publishDate | 2024-01-01 |
publisher | IOP Publishing |
record_format | Article |
series | The Astrophysical Journal |
spelling | doaj.art-494f93ddc0a741aa8d221ca3efa1875d2024-02-13T13:05:51ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-01962211610.3847/1538-4357/ad1a10Chasing the Break: Tracing the Full Evolution of a Black Hole X-Ray Binary Jet with Multiwavelength Spectral ModelingConstanza Echiburú-Trujillo0https://orcid.org/0000-0001-8436-1847Alexandra J. Tetarenko1https://orcid.org/0000-0003-3906-4354Daryl Haggard2https://orcid.org/0000-0001-6803-2138Thomas D. Russell3https://orcid.org/0000-0002-7930-2276Karri I. I. Koljonen4https://orcid.org/0000-0002-9677-1533Arash Bahramian5https://orcid.org/0000-0003-2506-6041Jingyi Wang6https://orcid.org/0000-0002-1742-2125Michael Bremer7Joe Bright8https://orcid.org/0000-0002-7735-5796Piergiorgio Casella9David M. Russell10https://orcid.org/0000-0002-3500-631XDiego Altamirano11https://orcid.org/0000-0002-3422-0074M. Cristina Baglio12https://orcid.org/0000-0003-1285-4057Tomaso Belloni13Chiara Ceccobello14https://orcid.org/0000-0002-4767-9925Stephane Corbel15Maria Diaz Trigo16https://orcid.org/0000-0001-7796-4279Dipankar Maitra17https://orcid.org/0000-0003-1897-6872Aldrin Gabuya18https://orcid.org/0000-0003-1541-7557Elena Gallo19https://orcid.org/0000-0001-5802-6041Sebastian Heinz20Jeroen Homan21https://orcid.org/0000-0001-8371-2713Erin Kara22https://orcid.org/0000-0003-0172-0854Elmar Körding23Fraser Lewis24Matteo Lucchini25https://orcid.org/0000-0002-2235-3347Sera Markoff26https://orcid.org/0000-0001-9564-0876Simone Migliari27James C. A. Miller-Jones28https://orcid.org/0000-0003-3124-2814Jerome Rodriguez29https://orcid.org/0000-0002-4151-4468Payaswini Saikia30https://orcid.org/0000-0002-5319-6620Craig L. Sarazin31https://orcid.org/0000-0003-0167-0981Tariq Shahbaz32https://orcid.org/0000-0003-1331-5442Gregory Sivakoff33https://orcid.org/0000-0001-6682-916XRoberto Soria34https://orcid.org/0000-0002-4622-796XVincenzo Testa35https://orcid.org/0000-0003-1033-1340Bailey E. Tetarenko36https://orcid.org/0000-0003-2636-6644Valeriu Tudose37Department of Astrophysical and Planetary Sciences, JILA, Duane Physics Bldg., 2000 Colorado Avenue, University of Colorado , Boulder, CO 80309, USA constanza.echiburu@colorado.edu; Department of Physics, McGill University , 3600 rue University, Montreal, Québec H3A 2T8, Canada; Trottier Space Institute , 3550 Rue University, Montréal, Québec H3A 2A7, CanadaDepartment of Physics and Astronomy, University of Lethbridge , Lethbridge, Alberta T1K 3M4, Canada; Department of Physics and Astronomy, Texas Tech University , Lubbock, TX 79409-1051, USA; East Asian Observatory, 660 N. A‘ohōkū Place, University Park , Hilo, HI 96720, USADepartment of Physics, McGill University , 3600 rue University, Montreal, Québec H3A 2T8, Canada; Trottier Space Institute , 3550 Rue University, Montréal, Québec H3A 2A7, CanadaINAF, Istituto di Astrofisica Spaziale e Fisica Cosmica , Via U. La Malfa 153, I-90146 Palermo, ItalyInstitutt for Fysikk, Norwegian University of Science and Technology , Høgskloreringen 5, Trondheim NO-7491, Norway; Finnish Centre for Astronomy with ESO (FINCA), University of Turku , Väisäläntie 20, FI-21500 Piikkiö, Finland; Aalto University , Metsahovi Radio Observatory, P.O. Box 13000, FI-00076 Aalto, FinlandInternational Centre for Radio Astronomy Research, Curtin University , Bentley, WA 6102, AustraliaMIT Kavli Institute for Astrophysics and Space Research , MIT, 70 Vassar Street, Cambridge, MA 02139, USAInstitut de Radioastronomie Millimétrique , 300 Rue de la Piscine, F-38406 Saint Martin d’Hères, FranceAstrophysics, Department of Physics, University of Oxford , Keble Road, Oxford OX1 3RH, UKINAF—Osservatorio Astronomico di Roma , Via Frascati 33, I-00078 Monteporzio Catone, ItalyCenter for Astrophysics and Space Science (CASS), New York University Abu Dhabi , P.O. Box 129188, Abu Dhabi, UAESchool of Physics and Astronomy, University of Southampton , Southampton SO17 1BJ, UKINAF-Osservatorio Astronomico di Brera , Via Bianchi 46, I-23807 Merate (LC), ItalyINAF-Osservatorio Astronomico di Brera , Via Bianchi 46, I-23807 Merate (LC), ItalyDepartment of Space, Earth and Environment, Chalmers University of Technology , Onsala Space Observatory, SE-439 92 Onsala, SwedenUniversité Paris-Saclay , Université Paris-Cité, CEA, CNRS, AIM, F-91191 Gif-sur-Yvette, FranceESO , Karl-Schwarzschild-Strasse 2, D-85748 Garching bei München, GermanyDepartment of Physics and Astronomy, Wheaton College , Norton, MA 02766, USAAl Sadeem Observatory , Al Wathba South, Abu Dhabi, UAE; Rizal Technological University , Mandaluyong City, PhilippinesDepartment of Astronomy, University of Michigan , 1085 South University Avenue, Ann Arbor, MI 48109, USADepartment of Astronomy, University of Wisconsin Madison , 475 N. Charter Street, Madison, WI 53706, USAEureka Scientific, Inc. , 2452 Delmer Street, Oakland, CA 94602, USAMIT Kavli Institute for Astrophysics and Space Research , MIT, 70 Vassar Street, Cambridge, MA 02139, USADepartment of Astrophysics/IMAPP, Radboud University , P.O. Box 9010, 6500 GL Nijmegen, The NetherlandsFaulkes Telescope Project, School of Physics and Astronomy, Cardiff University , The Parade, Cardiff CF24 3AA, Wales, UK; Astrophysics Research Institute, Liverpool John Moores University , 146 Brownlow Hill, Liverpool L3 5RF, UKMIT Kavli Institute for Astrophysics and Space Research , MIT, 70 Vassar Street, Cambridge, MA 02139, USA; Anton Pannekoek Institute for Astronomy, University of Amsterdam , Science Park 904, Amsterdam NL-1098 XH, The Netherlands; SRON Netherlands Institute for Space Research , Niels Bohrweg 4, 2333CA Leiden, The NetherlandsAnton Pannekoek Institute for Astronomy, University of Amsterdam , Science Park 904, Amsterdam NL-1098 XH, The Netherlands; Gravitation Astroparticle Physics Amsterdam (GRAPPA) Institute, University of Amsterdam , Science Park NL-904, Amsterdam 1098 XH, The NetherlandsAurora Technology , Calle Principe de Vergara, 211, 1-B, E-28002 Madrid, SpainInternational Centre for Radio Astronomy Research, Curtin University , Bentley, WA 6102, AustraliaUniversité Paris-Saclay , Université Paris-Cité, CEA, CNRS, AIM, F-91191 Gif-sur-Yvette, FranceCenter for Astrophysics and Space Science (CASS), New York University Abu Dhabi , P.O. Box 129188, Abu Dhabi, UAEDepartment of Astronomy, University of Virginia , 530 McCormick Road, Charlottesville, VA 22904-4325, USAInstituto de Astrofísica de Canarias (IAC) , E-38205 La Laguna, Tenerife, Spain; Departamento de Astrofísica, Universidad de La Laguna (ULL) , E-38206 La Laguna, Tenerife, SpainDepartment of Physics, University of Alberta , CCIS 4-181, Edmonton AB T6G 2E1, CanadaINAF, Osservatorio Astrofisico di Torino , Strada Osservatorio 20, I-10025 Pino Torinese, Italy; College of Astronomy and Space Sciences, University of the Chinese Academy of Sciences , Beijing 100049, People's Republic of China; Sydney Institute for Astronomy, School of Physics A28, The University of Sydney , Sydney, NSW 2006, AustraliaINAF—Osservatorio Astronomico di Roma , Via Frascati 33, I-00078 Monteporzio Catone, ItalyDepartment of Physics, McGill University , 3600 rue University, Montreal, Québec H3A 2T8, Canada; Trottier Space Institute , 3550 Rue University, Montréal, Québec H3A 2A7, CanadaInstitute for Space Sciences , Atomistilor 409, P.O. Box MG-23, 077125 Bucharest-Magurele, RomaniaBlack hole (BH) X-ray binaries (XRBs) are ideal targets to study the connection between accretion inflow and jet outflow. Here we present quasi-simultaneous, multiwavelength observations of the Galactic BH system MAXI J1820+070, throughout its 2018–2019 outburst. Our data set includes coverage from the radio through X-ray bands from 17 different instruments/telescopes, and encompasses 19 epochs over a 7 month period, resulting in one of the most well-sampled multiwavelength data sets of a BH XRB outburst to date. With our data, we compile and model the broadband spectra of this source using a phenomenological model that includes emission from the jet, a companion star, and an accretion flow. This modeling allows us to track the evolution of the spectral break in the jet spectrum, a key observable that samples the jet launching region. We find that the spectral break location changes over at least ≈3 orders of magnitude in electromagnetic frequency over this period. Using these spectral break measurements, we link the full cycle of jet behavior, including the rising, quenching, and reignition, to the changing accretion flow properties as the source evolves through its different accretion states. Our analysis shows consistent jet behavior with other sources in similar phases of their outbursts, reinforcing the idea that jet quenching and recovery may be a global feature of BH XRB systems in outburst. Our results also provide valuable evidence supporting a close connection between the geometry of the inner accretion flow and the base of the jet.https://doi.org/10.3847/1538-4357/ad1a10X-ray binary starsLow-mass x-ray binary starsRadio jets |
spellingShingle | Constanza Echiburú-Trujillo Alexandra J. Tetarenko Daryl Haggard Thomas D. Russell Karri I. I. Koljonen Arash Bahramian Jingyi Wang Michael Bremer Joe Bright Piergiorgio Casella David M. Russell Diego Altamirano M. Cristina Baglio Tomaso Belloni Chiara Ceccobello Stephane Corbel Maria Diaz Trigo Dipankar Maitra Aldrin Gabuya Elena Gallo Sebastian Heinz Jeroen Homan Erin Kara Elmar Körding Fraser Lewis Matteo Lucchini Sera Markoff Simone Migliari James C. A. Miller-Jones Jerome Rodriguez Payaswini Saikia Craig L. Sarazin Tariq Shahbaz Gregory Sivakoff Roberto Soria Vincenzo Testa Bailey E. Tetarenko Valeriu Tudose Chasing the Break: Tracing the Full Evolution of a Black Hole X-Ray Binary Jet with Multiwavelength Spectral Modeling The Astrophysical Journal X-ray binary stars Low-mass x-ray binary stars Radio jets |
title | Chasing the Break: Tracing the Full Evolution of a Black Hole X-Ray Binary Jet with Multiwavelength Spectral Modeling |
title_full | Chasing the Break: Tracing the Full Evolution of a Black Hole X-Ray Binary Jet with Multiwavelength Spectral Modeling |
title_fullStr | Chasing the Break: Tracing the Full Evolution of a Black Hole X-Ray Binary Jet with Multiwavelength Spectral Modeling |
title_full_unstemmed | Chasing the Break: Tracing the Full Evolution of a Black Hole X-Ray Binary Jet with Multiwavelength Spectral Modeling |
title_short | Chasing the Break: Tracing the Full Evolution of a Black Hole X-Ray Binary Jet with Multiwavelength Spectral Modeling |
title_sort | chasing the break tracing the full evolution of a black hole x ray binary jet with multiwavelength spectral modeling |
topic | X-ray binary stars Low-mass x-ray binary stars Radio jets |
url | https://doi.org/10.3847/1538-4357/ad1a10 |
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