Through observations in the near infrared range we've discovered that MHO 2147 has a captivating S shaped structure. This unique shape is thought to be the result of changes in direction over time possibly influenced by forces from neighboring celestial bodies acting on the central star. Despite these shifts the jet remains intact due to an emission from its core.
The region surrounding MHO 2147/8 is teeming with activity. We've identified two jets; MHO 2148 and a recently found third one situated next to MHO 2147. It's worth noting that MHO 2148 is positioned perpendicular to MHO 2147 suggesting dynamics within interstellar space.
At the heart of this system lies a triple star system known as IRAS 17527 2439 concealed within an opaque dark cloud. The high concentration of dust within this necessitates infrared observations for studying these celestial phenomena.
The accompanying image presents a composite infrared capture taken by the Gemini South Telescope in Chile offering us a mesmerizing glimpse, into the fascinating world of the MHO 2147/8 system.
The breathtaking picture captures the awe inspiring beauty of this cosmic marvel by utilizing a combination of broadband and narrow band filters that emphasize the emission of molecular hydrogen.
Credit image - International Gemini Observatory/NOIRLab/NSF/AURA with special thanks to PI; L. Ferrero from Universidad Nacional de Córdoba, for their contributions.
Post a Comment