ALMA’s view of the outflow associated with the Herbig-Haro object HH 46/47
Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have obtained a vivid close-up view of material streaming away from a newborn star. By looking at the glow coming from carbon monoxide molecules in an object called Herbig-Haro 46/47 they have discovered that its jets are even more energetic than previously thought. In these observations from ALMA the colours shown represent the motions of the material: the blue parts at the left are a jet approaching the Earth (blueshifted) and the larger jet on the right is receding (redshifted).
Źródło:ESO/ALMA (ESO/NAOJ/NRAO)/H. Arce
O zdjęciu
Identyfikator: | eso1336b |
Typ: | Obserwacje |
Data publikacji: | 20 sierpnia 2013 16:00 |
Powiązane komunikaty: | eso1336 |
Rozmiar: | 523 x 382 px |
O obiekcie
Nazwa: | HH 46, HH 47 |
Typ: | Milky Way : Star : Circumstellar Material : Outflow |
Odległość: | 1400 lat świetlnych |
Constellation: | Vela |
Kategoria: | Stars |
Współrzędne
Pozycja (RA): | 8 25 40.71 |
Pozycja (Dec): | -51° 0' 58.03" |
Pole widzenia: | 4.32 x 3.15 arcminutes |
Orientacja: | North is 0.2° lewo of vertical |
Kolory i filtry
Pasmo | Długość fali | Teleskop |
---|---|---|
Milimetrowy CO | 2.6 mm | Atacama Large Millimeter/submillimeter Array |
Milimetrowy CO | 2.97 mm | Atacama Large Millimeter/submillimeter Array |
Milimetrowy CO | 3.0 mm | Atacama Large Millimeter/submillimeter Array |