The Musca molecular cloud: An interstellar symphony
Dr. Aris Tritsis and Prof. Konstantinos Tassis of the Department of Physics of the University of Crete have reported the first-ever discovery of normal modes in a molecular cloud, called Musca. This discovery has allowed the two researchers to precisely determine the physical dimensions of the cloud. Caption: The Musca cloud appears as a luminous source when seen in infrared light. Data for this image are from the European Space Agency’s Herschel Space Observatory. Musca is an isolated cloud seen from the Southern hemisphere and it is one of the most ordered molecular clouds observed. The main dense structure of Musca, inside which stars will eventually form, is surrounded by hair-like structures called striations. In a previous study, also by Aris Tritsis and Konstantinos Tassis (Tritsis & Tassis 2016, MNRAS, 462, 3602), it was found that the only viable mechanism that could account for the formation of striations was through the excitation of magnetic pressure waves. However, in the case of the isolated Musca, the waves creating striations were trapped setting up normal modes. Caption: Computer simulation of the Musca cloud, performed at the Metropolis HPC Facility of the Crete Center for Quantum Complexity and Nanotechnology (CCQCN) of the University of Crete. The colour scale denotes density of the gas in the cloud. Black lines threading the cloud almost at right angles to its plane are the magnetic field lines. Because of its needle-like appearance on the plane of the sky, Musca was considered to be the poster-child of an interstellar filament against which many theoretical models were put to the test. However, in contradiction to conventional wisdom the normal-mode analysis of striations has shown that Musca is in fact a sheet seen edge-on. Article: “Magnetic Seismology of Interstellar Gas Clouds: Unveiling a Hidden Dimension", A. Tritsis, K. Tassis, Science 360, 6389, pp.635-638 (2018). |
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