LMC-driven anisotropic boosts in stream--subhalo interactions Article Swipe
Arpit Arora
,
Nicolás Garavito-Camargo
,
Robyn E. Sanderson
,
Emily Cunningham
,
Andrew Wetzel
,
Nondh Panithanpaisal
,
Megan Barry
·
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2309.15998
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2309.15998
Dark Matter (DM) subhalos are predicted to perturb stellar streams; stream morphologies and dynamics can constrain the mass distribution of subhalos. Using FIRE-2 simulations of Milky Way-mass galaxies, we show that presence of a Large Magellanic Cloud (LMC)--analog significantly changes stream-subhalo encounter rates. Three key factors drive these changes. First, the LMC--analog brings in many subhalos, increasing encounter rates for streams near the massive satellite by up to 20--40%. Second, the LMC--analog displaces the host from its center-of-mass (inducing reflex motion), causing a north-south asymmetry in the density and radial velocity distribution of subhalos. This asymmetry results in encounter rates varying by 50--70% across the sky at the same distance. Finally, the LMC--mass satellite induces a density wake in the host's DM halo, further boosting the encounter rates near the LMC--analog. We also explore the influence of stream orbital properties, finding a 50% increase in encounters for streams moving retrograde to the LMC--analog's orbit in the opposite hemisphere. The dependence of encounter rates on stream location and orbit has important implications for where to search for new streams with spurs and gaps in the Milky Way.
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Metadata
- Type
- preprint
- Language
- en
- Landing Page
- http://arxiv.org/abs/2309.15998
- https://arxiv.org/pdf/2309.15998
- OA Status
- green
- Cited By
- 1
- References
- 23
- Related Works
- 10
- OpenAlex ID
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https://openalex.org/W4387210395Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.48550/arxiv.2309.15998Digital Object Identifier
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LMC-driven anisotropic boosts in stream--subhalo interactionsWork title
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preprintOpenAlex work type
- Language
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enPrimary language
- Publication year
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2023Year of publication
- Publication date
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2023-09-27Full publication date if available
- Authors
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Arpit Arora, Nicolás Garavito-Camargo, Robyn E. Sanderson, Emily Cunningham, Andrew Wetzel, Nondh Panithanpaisal, Megan BarryList of authors in order
- Landing page
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https://arxiv.org/abs/2309.15998Publisher landing page
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https://arxiv.org/pdf/2309.15998Direct link to full text PDF
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YesWhether a free full text is available
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greenOpen access status per OpenAlex
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https://arxiv.org/pdf/2309.15998Direct OA link when available
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Physics, Milky Way, Astrophysics, Local Group, Halo, Asymmetry, Sky, Galaxy, Large Magellanic Cloud, Astronomy, Quantum mechanicsTop concepts (fields/topics) attached by OpenAlex
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1Total citation count in OpenAlex
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.Way-mass | 26 |
| abstract_inverted_index.boosting | 124 |
| abstract_inverted_index.changes. | 48 |
| abstract_inverted_index.dynamics | 13 |
| abstract_inverted_index.increase | 143 |
| abstract_inverted_index.location | 165 |
| abstract_inverted_index.motion), | 80 |
| abstract_inverted_index.opposite | 156 |
| abstract_inverted_index.presence | 31 |
| abstract_inverted_index.streams; | 9 |
| abstract_inverted_index.subhalos | 3 |
| abstract_inverted_index.velocity | 90 |
| abstract_inverted_index.(inducing | 78 |
| abstract_inverted_index.LMC--mass | 112 |
| abstract_inverted_index.asymmetry | 84, 95 |
| abstract_inverted_index.constrain | 15 |
| abstract_inverted_index.displaces | 72 |
| abstract_inverted_index.distance. | 109 |
| abstract_inverted_index.encounter | 41, 57, 98, 126, 161 |
| abstract_inverted_index.galaxies, | 27 |
| abstract_inverted_index.important | 169 |
| abstract_inverted_index.influence | 135 |
| abstract_inverted_index.predicted | 5 |
| abstract_inverted_index.satellite | 64, 113 |
| abstract_inverted_index.subhalos, | 55 |
| abstract_inverted_index.subhalos. | 20, 93 |
| abstract_inverted_index.Magellanic | 35 |
| abstract_inverted_index.dependence | 159 |
| abstract_inverted_index.encounters | 145 |
| abstract_inverted_index.increasing | 56 |
| abstract_inverted_index.retrograde | 149 |
| abstract_inverted_index.LMC--analog | 51, 71 |
| abstract_inverted_index.hemisphere. | 157 |
| abstract_inverted_index.north-south | 83 |
| abstract_inverted_index.properties, | 139 |
| abstract_inverted_index.simulations | 23 |
| abstract_inverted_index.LMC--analog. | 130 |
| abstract_inverted_index.distribution | 18, 91 |
| abstract_inverted_index.implications | 170 |
| abstract_inverted_index.morphologies | 11 |
| abstract_inverted_index.(LMC)--analog | 37 |
| abstract_inverted_index.LMC--analog's | 152 |
| abstract_inverted_index.significantly | 38 |
| abstract_inverted_index.center-of-mass | 77 |
| abstract_inverted_index.stream-subhalo | 40 |
| cited_by_percentile_year.max | 94 |
| cited_by_percentile_year.min | 90 |
| countries_distinct_count | 0 |
| institutions_distinct_count | 7 |
| sustainable_development_goals[0].id | https://metadata.un.org/sdg/14 |
| sustainable_development_goals[0].score | 0.7200000286102295 |
| sustainable_development_goals[0].display_name | Life below water |
| citation_normalized_percentile.value | 0.63187755 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |