We investigate the stellar mass–black hole mass (
The Magellanic Stream is sculpted by its infall through the Milky Way’s circumgalactic medium, but the rates and directions of mass, momentum, and energy exchange through the stream-halo interface are relative unknowns critical for determining the origin and fate of the Stream. Complementary to large-scale simulations of LMC-SMC interactions, we apply new insights derived from idealized, high-resolution
- NSF-PAR ID:
- Publisher / Repository:
- DOI PREFIX: 10.3847
- Date Published:
- Journal Name:
- The Astrophysical Journal
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- Article No. 120
- Medium: X
- Sponsoring Org:
- National Science Foundation
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We investigate the stellar mass–black hole mass (
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The Large Magellanic Cloud (LMC) has an extensive H
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