Z Camelopardalis,UV image
Numéro d’image : 11885896
| Z Camelopardalis,far ultraviolet image. Z Camelopardalis (centre,white) is a double-star (binary) system. It is composed of a dead star (white dwarf) and a companion star. This is an exploding binary system,in which mass is transferred from the companion star to the white dwarf. When the white dwarf reaches its mass limit,it explodes. In this image clouds of ionised gas,the remnants of an explosion,(nova) are detected surrounding the white dwarf (at left and below). Such explosions usually occur either as recurrent small explosions (recurrent dwarf novae) or single large blasts (classical novae). Z Camelopardalis is thought to have undergone both types of explosions. Image obtained by the Galaxy Evolution Explorer on January 25 2004 | |
| Licence : | Droits gérés |
| Crédit: | Science Photo Library / NASA |
| Taille de l’image : | 3000 px × 3000 px |
| Model Release : | Non requis |
| Property Release : | Non requis |
| Restrictions : | - |
Prix pour cette image À partir de 45 €
Produit vendu
(Calendrier, Carte postale, Carte de vœux, Impression sur textile, Packaging etc)
À partir de 45 €
Usage commercial
(Affichage, Annonce presse, Annonce TV, Carte, Digital - hors rés. sociaux, Digital - rés. sociaux etc)
À partir de 45 €
Éditorial
(Digital, Journal, Livre, Livre pratique, Magazine, Télévision etc)
À partir de 60 €
Usage non-commercial
(Digital - hors rés. sociaux, Digital - rés. sociaux etc)
À partir de 120 €
Mots clés
- astronomie,
- astronomique,
- astrophysique,
- astrophysiques,
- binaire,
- bizarre,
- camelopardalis,
- compagnon,
- cosmologie,
- de l'espace,
- effondré,
- espace,
- étoile,
- étrange,
- exploser,
- explosion,
- gaz ionisé,
- girafe,
- image satellite,
- ionisé,
- mort,
- mort d'étoile,
- naine blanche,
- Nova,
- particulier,
- récurrent,
- science,
- stellaire,
- supernova,
- ultraviolet,
- UV