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

SCHNEITER, E. M.; J. REYES-ITURBIDE; P. F. VELÁZQUEZ; ESQUIVEL, A.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

WILEY-BLACKWELL PUBLISHING, INC

Lugar: Londres; Año: 2022 vol. 511 p. 3420 - 3420

0035-8711

70 is a giant superbubble (SB) produced by the stellar cluster LH 114. The dynamic of the stellar SB can be explained withhydrodynamic simulations. Ho we v er, the e xplanation of the observ ed X-ray luminosity is still a matter of debate. Observationsshow that this kind of superbubbles exhibits X-ray luminosities of the order of 10 35 erg s −1 , which cannot be explained by onlyconsidering the mechanical luminosity of the stellar components. Instead, theoretical models predict luminosities one order ofmagnitude 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 explainthe missing X-ray emission, lasting approximately 1000 yr. Also, the radiation produces an enhancement of the filamentarysuperbubble morphology and it increases the SB radius by ∼ 23 p