Accretion-induced variability links young stellar objects, white dwarfs, and black holes

Author:

Scaringi Simone1ORCID,Maccarone Thomas J.2ORCID,Körding Elmar3,Knigge Christian4ORCID,Vaughan Simon5,Marsh Thomas R.6,Aranzana Ester3ORCID,Dhillon Vikram S.78ORCID,Barros Susana C. C.9

Affiliation:

1. Max-Planck-Institut für Extraterrestriche Physik, D-85748 Garching, Germany.

2. Department of Physics, Texas Tech University, Box 41051, Lubbock, TX 79409–1051, USA.

3. Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University Nijmegen, P. O. Box 9010, 6500 GL Nijmegen, Netherlands.

4. School of Physics and Astronomy, University of Southampton, Highfield, Southampton SO17 1BJ, UK.

5. Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK.

6. Department of Physics, University of Warwick, Coventry CV4 7AL, UK.

7. Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, UK.

8. Instituto de Astrofisica de Canarias, E-38205, La Laguna, Tenerife, Spain.

9. Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, Centro de Astrofísica da Universidade do Porto (CAUP), Rua das Estrelas, PT4150-762 Porto, Portugal.

Abstract

Astrophysical accretion is a universal process in objects from proto-stars to supermassive black holes.

Funder

Alexander von Humboldt-Stiftung

Science and Technology Facilities Council

Nederlandse Organisatie voor Wetenschappelijk Onderzoek

Fundação para a Ciência e a Tecnologia

Goddard Space Flight Center

National Aeronautics and Space Administration

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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