Anatomy of a Fall: Stationary and super-Keplerian spiral arms generated by accretion streamers in protostellar discs
Title: | Anatomy of a Fall: Stationary and super-Keplerian spiral arms generated by accretion streamers in protostellar discs |
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Authors: | Calcino, Josh, Price, Daniel J., Hilder, Thomas, Christiaens, Valentin, Speedie, Jessica, Ormel, Chris W. |
Publication Year: | 2024 |
Collection: | Astrophysics |
Subject Terms: | Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics |
More Details: | Late-stage infall onto evolved protoplanetary discs is an important source of material and angular momentum replenishment, and disc substructures. In this paper we used 3D smoothed particle hydrodynamics simulations to model streamer-disc interactions for a prograde streamer. The initially parabolic streamer interacts with the disc material to excite disc eccentricity, which can last on the order of $10^5$ years. We found that the spiral arms the streamer excited in the disc can have a variety of pattern speeds, ranging from stationary to super-Keplerian. Spiral arms with various pattern speeds can exist simultaneously, providing a way to diagnose them in observations. Streamer induced spirals appear similar to those generated by a massive outer companion, where the pitch angle of the spiral increases towards the source of the perturbation. Additionally, the spirals arms can show large and sudden pitch angle changes. Streamer induced spirals are long-lived, lasting approximately $3-4\times$ longer than the initial streamer infall timescale ($\sim$$10^4$ years). After the initial interaction with the disc, a long lasting low $m$ azimuthal mode persists in the disc. Comment: 12 pages, 11 figures, acception version |
Document Type: | Working Paper |
Access URL: | http://arxiv.org/abs/2410.18521 |
Accession Number: | edsarx.2410.18521 |
Database: | arXiv |
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Header | DbId: edsarx DbLabel: arXiv An: edsarx.2410.18521 RelevancyScore: 1112 AccessLevel: 3 PubType: Report PubTypeId: report PreciseRelevancyScore: 1112.27160644531 |
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Items | – Name: Title Label: Title Group: Ti Data: Anatomy of a Fall: Stationary and super-Keplerian spiral arms generated by accretion streamers in protostellar discs – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Calcino%2C+Josh%22">Calcino, Josh</searchLink><br /><searchLink fieldCode="AR" term="%22Price%2C+Daniel+J%2E%22">Price, Daniel J.</searchLink><br /><searchLink fieldCode="AR" term="%22Hilder%2C+Thomas%22">Hilder, Thomas</searchLink><br /><searchLink fieldCode="AR" term="%22Christiaens%2C+Valentin%22">Christiaens, Valentin</searchLink><br /><searchLink fieldCode="AR" term="%22Speedie%2C+Jessica%22">Speedie, Jessica</searchLink><br /><searchLink fieldCode="AR" term="%22Ormel%2C+Chris+W%2E%22">Ormel, Chris W.</searchLink> – Name: DatePubCY Label: Publication Year Group: Date Data: 2024 – Name: Subset Label: Collection Group: HoldingsInfo Data: Astrophysics – Name: Subject Label: Subject Terms Group: Su Data: <searchLink fieldCode="DE" term="%22Astrophysics+-+Earth+and+Planetary+Astrophysics%22">Astrophysics - Earth and Planetary Astrophysics</searchLink><br /><searchLink fieldCode="DE" term="%22Astrophysics+-+Astrophysics+of+Galaxies%22">Astrophysics - Astrophysics of Galaxies</searchLink><br /><searchLink fieldCode="DE" term="%22Astrophysics+-+Solar+and+Stellar+Astrophysics%22">Astrophysics - Solar and Stellar Astrophysics</searchLink> – Name: Abstract Label: Description Group: Ab Data: Late-stage infall onto evolved protoplanetary discs is an important source of material and angular momentum replenishment, and disc substructures. In this paper we used 3D smoothed particle hydrodynamics simulations to model streamer-disc interactions for a prograde streamer. The initially parabolic streamer interacts with the disc material to excite disc eccentricity, which can last on the order of $10^5$ years. We found that the spiral arms the streamer excited in the disc can have a variety of pattern speeds, ranging from stationary to super-Keplerian. Spiral arms with various pattern speeds can exist simultaneously, providing a way to diagnose them in observations. Streamer induced spirals appear similar to those generated by a massive outer companion, where the pitch angle of the spiral increases towards the source of the perturbation. Additionally, the spirals arms can show large and sudden pitch angle changes. Streamer induced spirals are long-lived, lasting approximately $3-4\times$ longer than the initial streamer infall timescale ($\sim$$10^4$ years). After the initial interaction with the disc, a long lasting low $m$ azimuthal mode persists in the disc.<br />Comment: 12 pages, 11 figures, acception version – Name: TypeDocument Label: Document Type Group: TypDoc Data: Working Paper – Name: URL Label: Access URL Group: URL Data: <link linkTarget="URL" linkTerm="http://arxiv.org/abs/2410.18521" linkWindow="_blank">http://arxiv.org/abs/2410.18521</link> – Name: AN Label: Accession Number Group: ID Data: edsarx.2410.18521 |
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RecordInfo | BibRecord: BibEntity: Subjects: – SubjectFull: Astrophysics - Earth and Planetary Astrophysics Type: general – SubjectFull: Astrophysics - Astrophysics of Galaxies Type: general – SubjectFull: Astrophysics - Solar and Stellar Astrophysics Type: general Titles: – TitleFull: Anatomy of a Fall: Stationary and super-Keplerian spiral arms generated by accretion streamers in protostellar discs Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Calcino, Josh – PersonEntity: Name: NameFull: Price, Daniel J. – PersonEntity: Name: NameFull: Hilder, Thomas – PersonEntity: Name: NameFull: Christiaens, Valentin – PersonEntity: Name: NameFull: Speedie, Jessica – PersonEntity: Name: NameFull: Ormel, Chris W. IsPartOfRelationships: – BibEntity: Dates: – D: 24 M: 10 Type: published Y: 2024 |
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