The star cluster Westerlund 1and the positions of the magnetar and its probable former companion star
This image of the young star cluster Westerlund 1 was taken with the Wide Field Imager on the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile. Although most stars in the cluster are hot blue supergiants, they appear reddish in this image as they are seen through interstellar dust and gas. European astronomers have for the first time demonstrated that the magnetar in this cluster — an unusual type of neutron star with an extremely strong magnetic field — probably was formed as part of a binary star system. The discovery of the magnetar’s former companion (Westerlund 1-5) elsewhere in the cluster helps solve the mystery of how a star that started off so massive could become a magnetar, rather than collapse into a black hole.
Źródło:ESO
O zdjęciu
Identyfikator: | eso1415b |
Typ: | Kolaż |
Data publikacji: | 14 maja 2014 12:00 |
Powiązane komunikaty: | eso1415 |
Rozmiar: | 1261 x 1261 px |
O obiekcie
Nazwa: | Westerlund 1 |
Typ: | Milky Way : Star : Grouping : Cluster |
Odległość: | 15000 lat świetlnych |
Constellation: | Ara |
Kategoria: | Star Clusters |
Współrzędne
Pozycja (RA): | 16 47 4.02 |
Pozycja (Dec): | -45° 51' 4.96" |
Pole widzenia: | 4.99 x 4.99 arcminutes |
Orientacja: | North is 0.1° prawo of vertical |
Kolory i filtry
Pasmo | Długość fali | Teleskop |
---|---|---|
Optyczny B | 451 nm | MPG/ESO 2.2-metre telescope WFI |
Optyczny V | 539 nm | MPG/ESO 2.2-metre telescope WFI |
Optyczny R | 651 nm | MPG/ESO 2.2-metre telescope WFI |