Could the Magnetic Star HD 135348 Possess a Rigidly Rotating Magnetosphere?
Rahul Jayaraman, Swetlana Hubrig, Daniel L. Holdsworth, Markus, Sch\"oller, Silva J\"arvinen, Donald W. Kurtz, George R. Ricker

TL;DR
This study investigates whether the magnetic star HD 135348 has a rigidly rotating magnetosphere by combining photometric TESS data and spectropolarimetric observations, highlighting the potential of TESS for identifying magnetic stars.
Contribution
The paper presents the first characterization of HD 135348 as a potential RRM star using combined photometric and spectropolarimetric data, and explores machine learning for identifying similar stars.
Findings
HD 135348 likely hosts a centrifugal magnetosphere.
Spectropolarimetric data show a magnetic field consistent with RRM stars.
Lack of typical emission profiles may be due to limited rotational phase coverage.
Abstract
We report the detection and characterization of a new magnetospheric star, HD 135348, based on photometric and spectropolarimetric observations. The TESS light curve of this star exhibited variations consistent with stars known to possess rigidly rotating magnetospheres (RRMs), so we obtained spectropolarimetric observations using the Robert Stobie Spectrograph (RSS) on the Southern African Large Telescope (SALT) at four different rotational phases. From these observations, we calculated the longitudinal magnetic field of the star , as well as the Alfv\'en and Kepler radii, and deduced that this star contains a centrifugal magnetosphere. However, an archival spectrum does not exhibit the characteristic "double-horned" emission profile for H and the Brackett series that has been observed in many other RRM stars. This could be due to the insufficient…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
