SIMBAD references

2020ApJ...894...19R - Astrophys. J., 894, 19-19 (2020/May-1)

An isolated white dwarf with 317 s rotation and magnetic emission.

REDING J.S., HERMES J.J., VANDERBOSCH Z., DENNIHY E., KAISER B.C., MACE C.B., DUNLAP B.H. and CLEMENS J.C.

Abstract (from CDS):

We report the discovery of short-period photometric variability and modulated Zeeman-split hydrogen emission in SDSSJ125230.93-023417.72 (EPIC 228939929), a variable white dwarf star observed at long cadence in K2 Campaign 10. The behavior is associated with a magnetic (B = 5.0 MG) spot on the stellar surface, making the 317.278 s period a direct measurement of the stellar rotation rate. This object is therefore the fastest-rotating, apparently isolated (without a stellar companion) white dwarf yet discovered and the second found to exhibit chromospheric Balmer emission after GD 356, in which the emission has been attributed to a unipolar inductor mechanism driven by a possible rocky planet. We explore the properties and behavior of this object, and consider whether its evolution may hold implications for white dwarf mergers and their remnants.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): White dwarf stars - Magnetic variable stars - Extrasolar rocky planets - Stellar mergers - Stellar rotation

VizieR on-line data: <Available at CDS (J/ApJ/894/19): fig3.dat>

Simbad objects: 4

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