Issue |
A&A
Volume 686, June 2024
|
|
---|---|---|
Article Number | A111 | |
Number of page(s) | 16 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/202348354 | |
Published online | 03 June 2024 |
Feasibility of detecting shadows in disks induced by infall
1
Institut für Theoretische Physik und Astrophysik, Christian-Albrechts-Universität zu Kiel,
Leibnizstraße 15,
24118
Kiel,
Germany
e-mail: akrieger@astrophysik.uni-kiel.de
2
Niels Bohr Institute, University of Copenhagen,
Øster Voldgade 5,
1350
Copenhagen,
Denmark
e-mail: kueffmeier@nbi.ku.dk
3
Zentrum für Astronomie der Universität Heidelberg, Institut für Theoretische Astrophysik,
Albert-Ueberle-Straße 2,
69120
Heidelberg,
Germany
4
School of Natural Sciences, Center for Astronomy, University of Galway,
Galway
H91 CF50,
Ireland
Received:
23
October
2023
Accepted:
7
March
2024
Observations performed with high-resolution imaging techniques have revealed the existence of shadows in circumstellar disks that can be explained by the misalignment of an inner disk with respect to an outer one. The cause of misalignment, however, is still a matter of debate. In this study, we investigate the feasibility of observing shadows induced by one prominent scenario that may lead to misalignment, which involves the late infall of material onto a protostellar system. In particular, we used previously performed hydrodynamical simulations of such events and we generated flux maps in the visible, near-infrared, submillimeter, and millimeter wavelength ranges using Monte Carlo radiative transfer. Based on those results, we derived synthetic observations of these systems performed with the instruments SPHERE/VLT and ALMA, which we used as a basis for our subsequent analysis. We find that near-infrared observations with SPHERE are particularly well suited for detecting shadows via direct imaging alongside other features such as gaps, arcs, and streamers. On the contrary, performing a shadow detection based on reconstructed ALMA observations is very challenging due to the high sensitivity that is required for this task. Thus, in cases that allow for a detection, sophisticated analyses may be needed, for instance by the utilization of carefully constructed azimuthal profiles, aiding the search for potentially shallow shadows. Lastly, we conclude that a late infall-induced disk misalignment offers a plausible explanation for the emergence of shadows observed in various systems.
Key words: accretion, accretion disks / hydrodynamics / radiative transfer / protoplanetary disks / ISM: kinematics and dynamics
© 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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