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Binary Star PDS 144B in Scorpius has a Proplyd – Ionized Protoplanetary Disk
PDS 144B is part of a binary star system known as PDS 144, which is notable for being the first confirmed Herbig Ae/Be binary system (2012) where both stars drive jets. Herbig Ae/Be stars are a class of pre-main-sequence stars that are more massive than T Tauri stars and are characterized by their emission lines…
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Dimethyl Ether Detected in MWC 480 Protoplanetary Disk
Dimethy Ether was first synthesised in 1835. It is expected to be used in biofuels in the future. The MWC 480 protoplanetary disk is a subject of significant interest due to its complex structure and potential insights into planet formation processes. Star Characteristics Protoplanetary Disk Features Kinematic and Chemical Properties Overall, the MWC 480 protoplanetary disk…
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HH 48 NE Protoplanetary Disk Ices at High Disk Altitudes
“To explain the presence of ices at high disk altitudes, we propose two possible scenarios: a disk wind that entrains sufficient amounts of dust, thus blocking part of the stellar UV radiation, or vertical mixing that cycles enough ices into the upper disk layers to balance ice photodesorption.” HH 48 NE is a protostar located…
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Formalhaut A with First Asteroid Belt Seen Outside Solar System
Fomalhaut A is a bright star and was known to the Persian and Arabic Astronomers. The name of the star is Arabic and means “mouth of the fish”. It belongs to a Tripple Star System 25 light-years away from earth. Formalhaut A has several notable characteristics: Fomalhaut Dusty Debris Disk (MIRI Image), James Webb Telescope…
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HL Tau Protoplanetary Disk Contains More Water Than Earth
The observations show that there is at least three times more water in the inner disc of the young Sun-like star HL Tauri than in all of Earth’s oceans combined. HL Tau also called HL Tauri is a young T Tauri star located approximately 450 light-years away from earth in the Taurus Molecular Cloud. It…