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not contain enough gas to form new stars — studies have shown the galaxy to have an associated cloud of gas nearby, hinting at recent star formation, and a population of young stars. The gas cloud does not lie within the galaxy itself, but is still gravitationally bound to it — meaning that it will eventually fall back into the galaxy over time. Since the cloud is close by, it’s likely that the process that flung it outwards it is still ongoing. After studying the shape of the gas cloud, astronomers suspect the most likely cause of the ejection to be supernova explosions within the galaxy. The data to create this image was selected from the ESO archive as part of the Hidden
Treasure competition.
993:
not contain enough gas to form new stars — studies have shown the galaxy to have an associated cloud of gas nearby, hinting at recent star formation, and a population of young stars. The gas cloud does not lie within the galaxy itself, but is still gravitationally bound to it — meaning that it will eventually fall back into the galaxy over time. Since the cloud is close by, it’s likely that the process that flung it outwards it is still ongoing. After studying the shape of the gas cloud, astronomers suspect the most likely cause of the ejection to be supernova explosions within the galaxy. The data to create this image was selected from the ESO archive as part of the Hidden
Treasure competition.
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This image shows a dwarf galaxy in the southern constellation of
Phoenix named, for obvious reasons, the Phoenix Dwarf. The Phoenix Dwarf is unique in that it cannot be classified according to the usual scheme for dwarf galaxies; while its shape would label it as a spheroidal dwarf galaxy — which do
992:
This image shows a dwarf galaxy in the southern constellation of
Phoenix named, for obvious reasons, the Phoenix Dwarf. The Phoenix Dwarf is unique in that it cannot be classified according to the usual scheme for dwarf galaxies; while its shape would label it as a spheroidal dwarf galaxy — which do
163:
The gas cloud does not lie within the galaxy itself, but is still gravitationally bound to it — meaning that it will eventually fall back into the galaxy over time. Since the cloud is close by, it’s likely that the process that flung it outwards it is still ongoing. After studying the shape of the
159:
The
Phoenix Dwarf is unique in that it cannot be classified according to the usual scheme for dwarf galaxies; while its shape would label it as a spheroidal dwarf galaxy — which do not contain enough gas to form new stars — studies have shown the galaxy to have an associated cloud of gas nearby,
720:
233:"Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts and captions, are licensed under a
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This file contains additional information, probably added from the digital camera or scanner used to create or digitize it.
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This image shows a dwarf galaxy in the southern constellation of
Phoenix named, for obvious reasons, the Phoenix Dwarf.
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gas cloud, astronomers suspect the most likely cause of the ejection to be supernova explosions within the galaxy.
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If the file has been modified from its original state, some details may not fully reflect the modified file.
166:
The data to create this image was selected from the ESO archive as part of the Hidden
Treasure competition.
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The following pages on the
English Knowledge (XXG) use this file (pages on other projects are not listed):
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237:, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible."
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246:: You must provide a link (URL) to the original file and the authorship information if available.
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hinting at recent star formation, and a population of young stars.
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Add a one-line explanation of what this file represents
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Creative
Commons Attribution 4.0 International License
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Creative
Commons Attribution 4.0 International License
87:(5,773 × 3,995 pixels, file size: 9.06 MB, MIME type:
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Commons is a freely licensed media file repository.
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432:Creative Commons Attribution 4.0 International
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256:
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186:https://www.eso.org/public/images/potw1838a/
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797:The following other wikis use this file:
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535:bc52ad8d6455d8deadabb4f4ccf2fdede93fcb74
147:An explosive phoenix - Phoenix Dwarf.jpg
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317:Creative Commons Attribution 4.0
1015:Date and time of data generation
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298:Under the following conditions:
269:This file is licensed under the
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915:Карликовая галактика в Фениксе
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220:This media was created by the
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967:European Southern Observatory
860:Մասնակից:A.sargsian/Ավազարկղ3
274:Attribution 4.0 International
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1053:Karl-Schwarzschild-Strasse 2
358:Items portrayed in this file
850:Anexo:Galaxias más cercanas
176:17 September 2018, 06:00:00
1093:
931:Usage on tr.wikipedia.org
921:Usage on sr.wikipedia.org
911:Usage on ru.wikipedia.org
901:Usage on pt.wikipedia.org
891:Usage on pl.wikipedia.org
881:Usage on nl.wikipedia.org
871:Usage on it.wikipedia.org
856:Usage on hy.wikipedia.org
846:Usage on es.wikipedia.org
836:Usage on de.wikipedia.org
821:Usage on cs.wikipedia.org
811:Usage on ca.wikipedia.org
801:Usage on bs.wikipedia.org
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1018:06:00, 17 September 2018
745:11:19, 17 September 2018
715:21:45, 17 September 2018
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108:This is a file from the
830:Trpasličí galaxie Fénix
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112:. Information from its
935:Phoenix Cüce Galaksisi
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115:description page there
46:Size of this preview:
214:
1058:Garching bei München
978:An explosive phoenix
840:Phoenix-Zwerggalaxie
805:Patuljasta galaksija
547:determination method
229:Their website states
74:5,773 × 3,995 pixels
70:2,560 × 1,772 pixels
1040:Contact information
925:Патуљаста галаксија
293:– to adapt the work
52:Other resolutions:
1046:http://www.eso.org
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66:1,280 × 886 pixels
62:1,024 × 709 pixels
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1023:JPEG file comment
825:Trpasličí galaxie
793:Global file usage
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467:17 September 2018
416:copyright license
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32:Global file usage
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865:Գաճաճ գալակտիկա
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815:Galàxia nana
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782:Dwarf galaxy
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683:File history
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123:You can help
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22:File history
1073:IIM version
1001:Usage terms
986:Image title
972:Short title
905:Galáxia anã
732:Fabian RRRR
396:copyrighted
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145:Description
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694:Date/Time
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452:inception
203:Licensing
154:English:
1032:Keywords
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285:to share
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Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
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