Issue |
A&A
Volume 682, February 2024
|
|
---|---|---|
Article Number | A104 | |
Number of page(s) | 7 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/202348375 | |
Published online | 08 February 2024 |
Probing initial distributions of orbital eccentricity and disc misalignment via polar discs
1
Dipartimento di Fisica, Università degli Studi di Milano,
via Celoria 16,
20133
Milano,
Italy
e-mail: simone.ceppi@unimi.it
2
Univ. Grenoble Alpes, CNRS, IPAG,
38000
Grenoble,
France
3
School of Physics and Astronomy, Monash University,
Clayton,
VIC 3800,
Australia
4
Department of Physics and Astronomy, University of Exeter,
Stocker Road,
Exeter
EX4 4QL,
UK
Received:
24
October
2023
Accepted:
15
December
2023
In a population of multiple protostellar systems with discs, the sub-population of circumbinary discs whose orbital plane is highly misaligned with respect to the binary’s orbital plane constrains the initial distribution of orbital parameters of the whole population. We show that by measuring the polar disc fraction and the average orbital eccentricity in the polar discs, one can constrain the distributions of initial eccentricity and mutual inclination in multiple stellar systems at birth.
Key words: accretion, accretion disks / hydrodynamics / methods: analytical / methods: statistical / protoplanetary disks / binaries: close
© The Authors 2024
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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