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Cluster observations of an ELD aligned current at the dawn ANK of a burst bulk ow K. Snekvik1, S. Haaland1,4, N. stgaard1, H. Hasegawa2, R. Nakamura3, T. Takada3, F. Pitout4, H. R me5, B. Klecker4,

Nakamura, Department of Physics and Technology, University of Bergen, No. 1055, Bergen, Norway e-mail: r.Nakamura{at}begin.ac.no Abstract The observed activity of super flares as observed in the field and the simulation has been associated with their formation as binary systems. However, the mechanism of the interaction between the companion (that is, the accretion disk) and the host is still unclear. This paper describes an approach to studying the binary system of an ELD as a star birth cluster in the field and further demonstrates its effectiveness by combining a single ELD with a pair of pulsars. The stellar birth cluster is shown to form after the collapse of a previously unstable binary star system. The binary star system undergoes an evolution like the core-collapse shock from neutron capture, which occurs when star accretion disks collide. The formation rate and the stellar mass depend on the parameters assumed for the binary system, such as luminosity, eccentricity, and density. A timescale for star formation is derived that spans from years to centuries to account for the time needed for binary systems to form. Furthermore, the process of star formation is simulated as a process using non-hydrogen material as input. Finally, the simulated stellar birth cluster reveals the observed brightness variations and other properties of the super flares along their evolution, such as rotation period and the mass-loss rate. Super flares as high-energy astronomical phenomena are very difficult to observe (e.g., see reviews by Manner et al. 2000; Roe sch, 2000; Manner, 2002), primarily because of their large sizes, long periods, and wide range of brightness, which make it difficult to distinguish any single super flare from many others. We will focus on their formation and evolution during active evolution.

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PATA Norway chapter is a branch of the Pacific Asia Travel Association (PATA) based in Norway, which focuses on promoting travel and tourism in the Pacific Asia region.

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Any travel and tourism industry organization based in Norway, that wants to be a part of the PATA network, can file for PATA Norway chapter.

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To fill out PATA Norway chapter, organizations need to complete the membership application form, provide the required documents and pay the membership fees as outlined by PATA Norway chapter.

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The purpose of PATA Norway chapter is to facilitate and encourage cooperation, exchange of information, and business opportunities among travel and tourism organizations in Norway and the Pacific Asia region.

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The specific information that needs to be reported on PATA Norway chapter may depend on the membership level, but generally, organizations are required to provide basic contact details, business profile, and information about their involvement in the travel and tourism industry.

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The deadline to file PATA Norway chapter in 2023 is currently not available. Please refer to the official PATA Norway chapter website or contact their office for the most updated information.

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