A MeerKAT survey of nearby novalike cataclysmic variables

Accepted/In Press date: 10 June 2020

Published date: 22 June 2020

Additional Information: Funding Information: DMH acknowledges financial support from the National Research Foundation (NRF) and the South African Astronomical Observatory (SAAO). PAW kindly acknowledges financial support from the University of Cape Town and the NRF. MLP acknowledges financial support from the NRF and the Newton Fund. JCAM-J is the recipient of an Australian Research Council Future Fellowship (FT140101082), funded by the Australian government. This work was supported by the Oxford Centre for Astrophysical Surveys, which is funded through generous support from the Hintze Family Charitable Foundation. Funding Information: This work has used data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https:// www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. Funding Information: The authors thank LCOGT and its staff for their continued support of ASAS-SN. ASAS-SN is supported by NSF grant AST-1515927. Development of ASAS-SN has been supported by NSF grant AST-0908816, the Center for Cosmology and AstroParticle Physics at the Ohio State University, the Mt. Cuba Astronomical Foundation, and by George Skestos. Funding Information: This publication has used data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by NASA and the National Science Foundation. Funding Information: This publication has used data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by NASA. Funding Information: Some of the data used were obtained from the Mikulski Archive for Space Telescopes. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Publisher Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.

Keywords: X-rays: binaries, accretion, accretion discs, novae, cataclysmic variables, radio continuum: stars, stars: jets, white dwarfs

Local EPrints ID: 442111

URI: http://eprints.soton.ac.uk/id/eprint/442111

DOI: doi:10.1093/mnras/staa1747

ISSN: 1365-2966

PURE UUID: f61639f4-60cd-4ea6-b4a2-f906bdf5ca32

ORCID for D. R. A. Williams: orcid.org/0000-0001-7361-0246

Date deposited: 07 Jul 2020 16:49

Last modified: 16 Mar 2024 08:26