Document Type
Article
Publication Title
Astronomy and Astrophysics
Abstract
Using an extensive X-ray dataset, we analyzed the X-ray emission of the massive O-star Tr16-22, which was recently found to be magnetic. Its bright X-ray emission is found to be modulated with a 54d period. This timescale should represent the rotational timescale of the star, as it does for other magnetic massive stars. In parallel, new spectropolarimetric data confirm the published magnetic detection.
DOI
10.1051/0004-6361/201424416
Publication Date
2014
Recommended Citation
Nazé, Yaël; Wade, Gregg A.; and Petit, Véronique, "Modulated X-Ray Emission Of The Magnetic O8.5V-Star Tr16-22" (2014). Aerospace, Physics, and Space Science Faculty Publications. 180.
https://repository.fit.edu/apss_faculty/180