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HD 41534，又名CD-32 2743，SAO 196459、HR 2149，是一颗恒星，视星等为5.65，位于銀經238.43，銀緯-23.36，其B1900.0坐标为赤經6h 0m 37.1s，赤緯-32° -23.36′ 11″。
, HD 41534 är en dubbelstjärna i den mellers … HD 41534 är en dubbelstjärna i den mellersta delen av stjärnbilden Duvan. Den har en kombinerad skenbar magnitud av ca 5,65 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 3,5 mas, beräknas den befinna sig på ett avstånd på ca 950 ljusår (ca 290 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 93 km/s. Den är en flyktstjärna med en ovanligt stor egenrörelse av ca 188 km/s och har blivit utstött från OB-föreningen Sco OB1 för omkring 14 miljoner år sedan. Sco OB1 för omkring 14 miljoner år sedan.
, HD 41534 is a binary star system in the so … HD 41534 is a binary star system in the southern constellation of Columba. It is dimply visible to the naked eye with a combined apparent visual magnitude of 5.65. The distance to this system is approximately 950 light-years based on parallax, and it is receding from the Sun with a radial velocity of +93 km/s. This is a runaway star system with an unusually high peculiar velocity of 187.6+12.2−13.8 km/s. It is thought to have been ejected from the OB association Sco OB 1 approximately 14 million years ago. The primary component is a B-type main-sequence star with a stellar classification of B2V. It displays microvariability with an amplitude of 0.0086 in magnitude and a frequency of 0.11316 cycles per day. The star is an estimated 14 million years old with a high rate of spin, showing a projected rotational velocity of 122. It has seven times the mass of the Sun and about four times the Sun's radius. HD 41534 is radiating over 1,600 times the luminosity of the Sun from its photosphere at an effective temperature of 20,000 K.e at an effective temperature of 20,000 K.
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HD 41534 är en dubbelstjärna i den mellers … HD 41534 är en dubbelstjärna i den mellersta delen av stjärnbilden Duvan. Den har en kombinerad skenbar magnitud av ca 5,65 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 3,5 mas, beräknas den befinna sig på ett avstånd på ca 950 ljusår (ca 290 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 93 km/s. Den är en flyktstjärna med en ovanligt stor egenrörelse av ca 188 km/s och har blivit utstött från OB-föreningen Sco OB1 för omkring 14 miljoner år sedan. Sco OB1 för omkring 14 miljoner år sedan.
, HD 41534 is a binary star system in the so … HD 41534 is a binary star system in the southern constellation of Columba. It is dimply visible to the naked eye with a combined apparent visual magnitude of 5.65. The distance to this system is approximately 950 light-years based on parallax, and it is receding from the Sun with a radial velocity of +93 km/s. This is a runaway star system with an unusually high peculiar velocity of 187.6+12.2−13.8 km/s. It is thought to have been ejected from the OB association Sco OB 1 approximately 14 million years ago.o OB 1 approximately 14 million years ago.
, HD 41534，又名CD-32 2743，SAO 196459、HR 2149，是一颗恒星，视星等为5.65，位于銀經238.43，銀緯-23.36，其B1900.0坐标为赤經6h 0m 37.1s，赤緯-32° -23.36′ 11″。
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