Stars Born in the Wind: M82's Outflow and Halo Star Formation

TL;DR

This study investigates how starburst-driven outflows in M82 may trigger star formation in the galaxy's halo by analyzing stellar populations and their formation history over the past 500 million years.

Contribution

It provides the first detailed star formation history of M82's halo features, linking halo star formation to disk starburst activity and outflow interactions.

Findings

85% of halo stars formed 150-70 Myr ago

Star formation in the halo correlates with disk starburst timing

Two mechanisms for halo star formation are proposed

Abstract

Starburst galaxies, like M82, launch kiloparsec-scale galactic outflows that interact with the circumgalactic medium (CGM) in complex ways. Apart from enriching the CGM with metals and energy, these outflows may trigger star formation in the halo -- either by driving shocks into the CGM or transporting cold, star-forming gas. To investigate such processes, we analyze the star formation history (SFH) of the Southern Arcs -- arc-like stellar features located ~5 kpc from M82's star-forming disk along the minor axis -- using Hubble Space Telescope Wide Field Camera 3 photometry. From resolved stellar populations, we derive SFHs over the last ~500 Myr, finding that ~85% of the stellar mass formed between ~150 and ~70 Myr ago, followed by a brief pause, with the remaining ~15% forming since ~30 Myr ago. The two stellar populations are co-spatial on scales of at least ~200 pc. The timing of the ~100 Myr burst aligns with star formation in the M82 disk and the age distribution of its star clusters, suggesting a causal link between the disk starburst and halo star formation. We explore two mechanisms that could explain these observations. In the first, shocks driven by the interaction between hot outflowing gas and cooler CGM material compress dense clouds, triggering collapse and star formation. In the second, stars form directly within massive, cool clouds associated with the outflow. As these clouds move ballistically through the halo, subsequent interactions with tidal debris may trigger additional star formation, producing the observed episodic structure.