Issue |
A&A
Volume 696, April 2025
|
|
---|---|---|
Article Number | A49 | |
Number of page(s) | 12 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361/202453353 | |
Published online | 02 April 2025 |
Reconstruction of spider system’s observables from orbital-period modulations via the Applegate mechanism
1
Scuola Superiore Meridionale, Largo San Marcellino 10, 80138 Napoli, Italy
2
Istituto Nazionale di Fisica Nucleare (INFN), sez. di Napoli, Via Cinthia 9, I-80126 Napoli, Italy
3
INAF – Osservatorio Astronomico di Cagliari, Via della Scienza 5, I-09047 Selargius (CA), Italy
⋆ Corresponding authors; v.defalco@ssmeridionale.it, amodio.carleo@inaf.it, alessandro.ridolfi@inaf.it
Received:
9
December
2024
Accepted:
28
February
2025
Redback and black-widow pulsars are two classes of peculiar binary systems characterised by very short orbital periods, very low-mass companions, and, in several cases, regular eclipses in their pulsed radio signal. Long-term timing revealed systematic but unpredictable variations in the orbital period, which can most likely be explained by the so-called Applegate mechanism. This relies on the magnetic dynamo activity generated inside the companion star and triggered by the pulsar wind, which induces a modification of the star’s oblateness (or quadrupole variation). This, in turn, couples with the orbit by gravity, causing a consequent change in the orbital period. The Applegate description is limited to providing estimates of physical quantities by highlighting their orders of magnitude. Therefore, we derived the time-evolution differential equations underlying the Applegate model; that is, we tracked such physical quantities in terms of time. Our strategy is to employ the orbital period modulations, measured by fitting the observational data, and implement a highly accurate approximation scheme to finally reconstruct the dynamics of the spider system in question and the relative observables. Among the latter is the magnetic field activity inside the companion star, which is still a matter of debate for its complex theoretical modelling and the ensuing expensive numerical simulations. As an application, we exploited our methodology to examine two spider sources: 47 Tuc W (redback) and 47 Tuc O (black widow). In this paper, the results obtained are analysed and then discussed in relation to the literature.
Key words: dynamo / gravitation / magnetic fields / binaries: eclipsing
© The Authors 2025
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.
This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.