A MeerKAT survey of nearby nova-like cataclysmic variables

Autor: M. L. Pretorius, N. Castro Segura, Kunal Mooley, David R. Williams, Ian Heywood, Antonia Rowlinson, Benjamin Stappers, R. P. Armstrong, Ralph A. M. J. Wijers, Paul J. Groot, D. M. Hewitt, Vanessa McBride, A. J. van der Horst, Christian Knigge, Rob Fender, Elmar Koerding, Assaf Horesh, E. Tremou, James Miller-Jones, Patrick Woudt
Přispěvatelé: High Energy Astrophys. & Astropart. Phys (API, FNWI), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Jazyk: angličtina
Rok vydání: 2020
Předmět:
Astronomy
Astrophysics::High Energy Astrophysical Phenomena
FOS: Physical sciences
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
Power law
Luminosity
stars: jets
X-rays: binaries
accretion
0103 physical sciences
Astrophysics::Solar and Stellar Astrophysics
010303 astronomy & astrophysics
Solar and Stellar Astrophysics (astro-ph.SR)
Astrophysics::Galaxy Astrophysics
white dwarfs
Physics
novae
High Energy Astrophysical Phenomena (astro-ph.HE)
cataclysmic variables
Accretion (meteorology)
010308 nuclear & particles physics
Spectral density
White dwarf
Astronomy and Astrophysics
Nova (laser)
accretion discs
Neutron star
Astrophysics - Solar and Stellar Astrophysics
Space and Planetary Science
System parameters
Astrophysics - High Energy Astrophysical Phenomena
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
radio continuum: stars
Zdroj: Monthly Notices of the Royal Astronomical Society, 496(3), 2542-2557. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 496, 2542-2557
Monthly Notices of the Royal Astronomical Society, 496, 3, pp. 2542-2557
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 496 (3), pp.2542-2557. ⟨10.1093/mnras/staa1747⟩
ISSN: 0035-8711
1365-2966
DOI: 10.1093/mnras/staa1747⟩
Popis: We present the results of MeerKAT radio observations of eleven nearby novalike cataclysmic variables. We have detected radio emission from IM Eri, RW Sex, V3885 Sgr and V603 Aql. While RW Sex, V3885 Sgr and V603 Aql had been previously detected, this is the first reported radio detection of IM Eri. Our observations have doubled the sample of non-magnetic CVs with sensitive radio data. We observe that at our radio detection limits, a specific optical luminosity $\gtrsim 2.2\times 10^{18}$ erg/s/Hz (corresponding to $M_V \lesssim 6.0$) is required to produce a radio detection. We also observe that the X-ray and radio luminosities of our detected novalikes are on an extension of the $L_{X} \propto L_{R}^{\sim 0.7}$ power law originally proposed for non-pulsating neutron star low-mass X-ray binaries. We find no other correlations between the radio emission and emission in other wavebands or any other system parameters for the existing sample of radio-detected non-magnetic CVs. We measure in-band (0.9-1.7 GHz) radio spectral indices that are consistent with reports from earlier work. Finally, we constructed broad spectral energy distributions for our sample from published multi-wavelength data, and use them to place constraints on the mass transfer rates of these systems.
Comment: 16 pages, 9 figures, accepted to MNRAS
Databáze: OpenAIRE