# A Jansky VLA Survey of Magnetic Cataclysmic Variable Stars: I. The Data

**Authors:** Paul E. Barrett, Christopher Dieck, Anthony J. Beasley, Kulinder P., Singh, and Paul A. Mason

arXiv: 1702.07631 · 2017-12-06

## TL;DR

This study used the Jansky VLA to observe 121 magnetic cataclysmic variables, detecting 19 in radio frequencies, with 14 being new sources, and identified two classes of radio emission mechanisms among these stars.

## Contribution

First comprehensive radio survey of magnetic cataclysmic variables, doubling known radio-emitting MCVs and proposing two distinct emission classes based on polarization.

## Key findings

- 19 stars detected in radio frequencies
- 14 new radio sources identified
- Two classes of radio emission suggested

## Abstract

The Jansky Very Large Array was used to observe 121 magnetic cataclysmic variables (MCVs). We report radio detections of 19 stars. Fourteen are new radio sources, increasing the number of MCVs that are radio sources by more than twofold, from 8 to 22. Most detections are at 8.7 GHz (X-band) with a lesser number at 5.4 and 21.1 GHz (C- and K-bands). Most flux density limits are in the range of 47-470 uJy. With the exception of AE Aqr, the maximum flux detected is 818 uJy. Fourteen of the detections show approximately 100% circularly polarized emission, which is characteristic of electron-cyclotron maser emission. The data suggest that MCVs might be divided into two classes of radio emitters: those dominated by weakly polarized gyro-synchrotron emission and those by highly polarized electron-cyclotron maser emission.

## Full text

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## Figures

3 figures with captions in the complete paper: https://tomesphere.com/paper/1702.07631/full.md

## References

20 references — full list in the complete paper: https://tomesphere.com/paper/1702.07631/full.md

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Source: https://tomesphere.com/paper/1702.07631