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Young Star HH 211 with Bipolar Jets is a Source of Molecular Emission
HH 211 is a young bipolar protostellar outflow that provides insights into the early stages of star formation. Here are the key points about HH 211 from the search results: Molecular Emission HH 211 is a prominent source of molecular emission, particularly molecular hydrogen (H2), which traces the outflow’s shocked molecular gas. The molecular emission dominates…
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Very-Low-Mass Star ISO-Chal 147 with Abundant Hydrocarbons in Protoplanetary Disk
ISO-Chal-1471 is a young, low-mass star located approximately 600 light-years away from Earth. ISO-Chal 147 is located in the Chamaeleon I star-forming cloud. It is a red dwarf star, which is a type of star that is very common in the Milky Way and burns through fuel slowly. Here are the key points from recent…
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JWST Live Stream
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Use of chatGPT (AI System) in Astronomy – an Example
Human: Could you analyze and structure the following text and create the content for a slide presentation out of it: “Young exoplanets are attractive targets for atmospheric characterization to explore the early phase of planetary evolution and the surrounding environment. Recent observations of the 10 Myr young Neptune-sized exoplanet K2-33b revealed that the planet’s transit…
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How to Download, View, And Edit Images from the James Webb Space Telescope with Jdaviz and Imviz
Like to comfortably view and edit images from the Jamew Webb Space Telescope like an astronomer ? Then follow this step by step cheatsheet guides if you are using windows on a PC . Main Software Components There are three key software components required: Microsoft C++ 14 Jupyter Notebook (Python) Jdaviz Additonal MAST Token to…
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Circular Astronomy 