Anatomy of a Fall: Stationary and super-Keplerian spiral arms generated by accretion streamers in protostellar discs

Bibliographic Details
Title: Anatomy of a Fall: Stationary and super-Keplerian spiral arms generated by accretion streamers in protostellar discs
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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  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>
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  Label: Publication Year
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  Data: 2024
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  Data: Astrophysics
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  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
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      – SubjectFull: Astrophysics - Earth and Planetary Astrophysics
        Type: general
      – SubjectFull: Astrophysics - Astrophysics of Galaxies
        Type: general
      – SubjectFull: Astrophysics - Solar and Stellar Astrophysics
        Type: general
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      – TitleFull: Anatomy of a Fall: Stationary and super-Keplerian spiral arms generated by accretion streamers in protostellar discs
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