Non-thermal radio emission from colliding flows in classical nova V1723 Aql

Jennifer H.S. Weston, J. L. Sokoloski, Brian D. Metzger, Yong Zheng, Laura Chomiuk, Miriam I. Krauss, Justin D. Linford, Thomas Nelson, Amy J. Mioduszewski, Michael P. Rupen, Tom Finzell, Koji Mukai

Research output: Contribution to journalArticlepeer-review

19 Scopus citations

Abstract

The importance of shocks in nova explosions has been highlighted by Fermi's discovery of γ -ray-producing novae. Over three years of multiband Very Large Array radio observations of the 2010 nova V1723 Aql show that shocks between fast and slow flows within the ejecta led to the acceleration of particles and the production of synchrotron radiation. Soon after the start of the eruption, shocks in the ejecta produced an unexpected radio flare, resulting in a multipeaked radio light curve. The emission eventually became consistent with an expanding thermal remnant with mass 2 × 10-4M and temperature 104 K. However, during the first two months, the ≥106 K brightness temperature at low frequencies was too high to be due to thermal emission from the small amount of X-ray-producing shock-heated gas. Radio imaging showed structures with velocities of 400 km s-1 (d/6 kpc) in the plane of the sky, perpendicular to a more elongated 1500 km s-1 (d/6 kpc) flow. The morpho-kinematic structure of the ejecta from V1723 Aql appears similar to nova V959 Mon, where collisions between a slow torus and a faster flow collimated the fast flow and gave rise to γ -ray-producing shocks. Optical spectroscopy and X-ray observations of V1723 Aql during the radio flare are consistent with this picture. Our observations support the idea that shocks in novae occur when a fast flow collides with a slow collimating torus. Such shocks could be responsible for hard X-ray emission, γ -ray production, and double-peaked radio light curves from some classical novae.

Original languageEnglish (US)
Pages (from-to)887-901
Number of pages15
JournalMonthly Notices of the Royal Astronomical Society
Volume457
Issue number1
DOIs
StatePublished - Jan 11 2016

Bibliographical note

Publisher Copyright:
© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.

Keywords

  • Binaries: general
  • Novae, cataclysmic variables
  • Radio continuum: stars
  • Stars: variables: general
  • Stars: winds, outflows
  • White dwarfs

Fingerprint

Dive into the research topics of 'Non-thermal radio emission from colliding flows in classical nova V1723 Aql'. Together they form a unique fingerprint.

Cite this