Amb motiu del tancament d'estiu, la validació de documents es reprendrà a partir del 28 d'agost de 2026. Disculpeu les molèsties.
Con motivo del cierre de verano, la validación de documentos se reanudará a partir del 28 de agosto de 2026. Disculpad las molestias
Due to the summer closure, document validation will resume starting August 28, 2026. We apologize for any inconvenience.

Document type

Bachelor thesis

Publication date

Publication license

cc-by-nc-nd (c) Gutiérrez, 2023
Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/201115

New orbital solution for LS 5039 and search for period variability

Journal Title

Director/Tutor

Journal ISSN

Volume Title

Related resource

Abstract

In recent decades, the study of high-energy gamma-ray emitting astrophysical objects has led to the discovery of a new type of object called gamma-ray emitting binaries (GREB). Among the approximately 30 known GREBs, several consist of a compact object and a massive star. The ones characterised by having the peak of their spectral energy distribution at >∼ 1 MeV are called gamma-ray binaries (γBs). So far, ten γBs, including LS 5039, have been confirmed as sources of high and/or very high-energy γ-ray emission. Understanding the physical processes of binary systems like LS 5039 is crucial. As their behaviour depends on the orbital phase, obtaining comprehensive information about the orbital parameters and their potential evolution is of great importance. In this work, we report the study of the evolution of the orbital period of LS 5039 through the fitting of orbital solutions to radial velocities using the program Spectroscopy Binary Orbit Program (SBOP). Our study revealed no significant variation within the observed time frame. The new orbital solution we derived, Porb = 3.90599 ± 0.00002 day, is an order of magnitude more precise than the previous solution. Additionally, we assessed the potential impact of energy loss due to the emission of gravitational waves on the orbital period evolution, concluding that it was too small to significantly influence the results

Description

Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2023, Tutor: Marc Ribó Gomis

Citation

Citation

GUTIÉRREZ LÜTKEN, Gunnar. New orbital solution for LS 5039 and search for period variability. [consulted: 8 of August of 2026]. Available at: https://hdl.handle.net/2445/201115

Export metadata

JSON - METS

Share record