Modelling the compact jet in MAXI J1836-194 with disc-driven shocks-Reference-Cited by-同舟云学术

Modelling the compact jet in MAXI J1836-194 with disc-driven shocks

Published:2018-10-17 Issue:2 Volume:482 Page:2447-2458
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Péault M¹^ORCID,Malzac J¹,Coriat M¹,Russell T D²^ORCID,Koljonen K I I³⁴⁵^ORCID,Belmont R¹⁶,Corbel S⁶⁷,Drappeau S¹,Ferreira J⁸,Petrucci P O⁸,Rodriguez J⁶,Russell D M⁵^ORCID

Affiliation:

1. IRAP, Université de Toulouse, CNRS, UPS, CNES, Toulouse, France

2. Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, NL-1098 XH Amsterdam, the Netherlands

3. Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Väisäläntie 20, FI-21500 Piikkiö, Finland

4. Aalto University Metsähovi Radio Observatory, PO Box 13000, FI-00076 Aalto, Finland

5. New York University Abu Dhabi, PO Box 129188, Abu Dhabi, UAE

6. Laboratoire AIM (CEA/IRFU - CNRS/INSU - Universitë Paris Diderot), CEA DRF/IRFU/DAp, F-91191 Gif-sur-Yvette, France

7. Station de Radioastronomie de Nançay, Observatoire de Paris, PSL Research University, CNRS, Univ. Orléans, F- Nançay, France

8. Université Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France

Funder

French Research National Agency

National Aeronautics and Space Administration

Netherlands Organisation for Scientific Research

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/482/2/2447/26575888/sty2796.pdf

Reference51 articles.

1. The acceleration of cosmic rays in shock fronts - I

2. Relativistic jets as compact radio sources

3. Hydromagnetic flows from accretion discs and the production of radio jets

4. “Soft X-ray transient” outbursts which are not soft

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