X-ray and optical emission from large superbubbles including the stellar photoionization

Author:

Schneiter E M12ORCID,Reyes-Iturbide J3,Velázquez P F4,Esquivel A4ORCID

Affiliation:

1. Instituto de Astronomía Teórica y Experimental-CONICET , Laprida 854, Córdoba X5000BGR , Argentina

2. Departamento de Materiales y Tecnologia , FCEFyN-UNC, Av. Vélez Sarsfield 1611, Córdoba X5016GCA , Argentina

3. Divisón de Mecánica, Tecnología de Estudios Superiores de Tianguistenco , Carretera Tenango La Marquesa Km 22, Santiago Tianguistenco, Estado de México , México

4. Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México , Apdo. Postal 70-543, 04510 Mexico City , México

Abstract

ABSTRACT N70 is a giant superbubble (SB) produced by the stellar cluster LH 114. The dynamic of the stellar SB can be explained with hydrodynamic simulations. However, the explanation of the observed X-ray luminosity is still a matter of debate. Observations show that this kind of superbubbles exhibits X-ray luminosities of the order of 1035 erg s−1, which cannot be explained by only considering the mechanical luminosity of the stellar components. Instead, theoretical models predict luminosities one order of magnitude lower. In this work, we attempt to answer this discrepancy by including a core-collapse supernova explosion (SN) and the photons emitted by each of the stars involved. We find that a core-collapse SN, with an initial mass of 10 M⊙, can explain the missing X-ray emission, lasting approximately 1000 yr. Also, the radiation produces an enhancement of the filamentary superbubble morphology and it increases the SB radius by $\sim 23{{\ \rm per\ cent}}$ with respect to the pure hydrodynamic case.

Funder

UNAM

George Mason University

University of Michigan

University of Cambridge

NASA

Goddard Space Flight Center

TNM

SEP

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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