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).
Crédit:ESO/ALMA (ESO/NAOJ/NRAO)/H. Arce
À propos de l'image
Identification: | eso1336b |
Type: | Observation |
Date de publication: | 20 août 2013 16:00 |
Communiqués de presse en rapport: | eso1336 |
Taille: | 523 x 382 px |
À propos de l'objet
Nom: | HH 46, HH 47 |
Type: | Milky Way : Star : Circumstellar Material : Outflow |
Distance: | 1400 années lumière |
Constellation: | Vela |
Catégorie: | Stars |
Fonds d'écran
Coordinates
Position (RA): | 8 25 40.71 |
Position (Dec): | -51° 0' 58.03" |
Field of view: | 4.32 x 3.15 arcminutes |
Orientation: | North is 0.2° left of vertical |
Couleurs & filtres
Domaine | Longueur d'onde | Télescope |
---|---|---|
Millimétrique CO | 2.6 mm | Atacama Large Millimeter/submillimeter Array |
Millimétrique CO | 2.97 mm | Atacama Large Millimeter/submillimeter Array |
Millimétrique CO | 3.0 mm | Atacama Large Millimeter/submillimeter Array |