New Frontiers in the Study of Magnetic Massive Stars with the Habitable Worlds Observatory

TL;DR

This paper discusses how the Pollux spectropolarimeter on the Habitable Worlds Observatory will revolutionize the study of magnetic massive stars, providing insights into their evolution and role in cosmic history.

Contribution

It introduces the Pollux instrument on HWO as a novel tool to advance understanding of magnetic fields in massive stars beyond current observational limits.

Findings

Pollux will enable detection of magnetic fields in distant massive stars.

It will provide data to understand magnetic influence on stellar evolution.

The instrument will impact studies of stellar feedback and compact objects.

Abstract

High-mass stars are notable for several reasons: they are characterized by strong winds, which inject momentum and enriched material into their surroundings, and die spectacularly as supernovae, leaving behind compact remnants and heavy elements (such as those that make life on Earth possible). Despite their relative rarity, they play a disproportionate role in the evolution of the galaxies that host them, and likely also played a significant role in the early days of the Universe. A subset ($\sim$10\%) of these stars was also found to host magnetic fields on their surface. These fields impact their evolution, and may lead to exotic physics (e.g., heavy stellar-mass black holes, pair-instability supernovae, magnetars, etc.). However, the detection and measurement of magnetic fields is limited, due to current instrumentation, to nearby massive stars in the Milky Way. To truly understand how magnetism arises in massive stars, and what role it might have played in earlier stages of our Universe, we require next-generation hardware, such as the proposed near-infrared-to-ultraviolet spectropolarimeter Pollux, on the Habitable Worlds Observatory (HWO). In this contribution, we detail how Pollux @ HWO will enable new frontiers in the study of magnetic massive stars, delivering results that will profoundly impact the fields of stellar formation, stellar evolution, compact objects, and stellar feedback.