User:Gsten03/sandbox
- These galaxies with lower luminosity are more likely to be found in clusters, such as the coma cluster, than in groups.
- Ultra diffuse galaxies have a similar size to the Milky Way, but they have masses more akin to dwarf galaxies.
- The formation of ultra diffuse galaxies is still debated, however they're thought to have formed from the earliest of galaxies or tidal forces.
 | This is a user sandbox of Gsten03. You can use it for testing or practicing edits. This is not the place where you work on your assigned article for a dashboard.wikiedu.org course. Visit your Dashboard course page and follow the links for your assigned article in the My Articles section. |
- Burg, Remco F. J. van der; Hoekstra, Henk; Muzzin, Adam; Sifón, Cristóbal; Viola, Massimo; Bremer, Malcolm N.; Brough, Sarah; Driver, Simon P.; Erben, Thomas; Heymans, Catherine; Hildebrandt, Hendrik; Holwerda, Benne W.; Klaes, Dominik; Kuijken, Konrad; McGee, Sean (2017-11-01). "The abundance of ultra-diffuse galaxies from groups to clusters - UDGs are relatively more common in more massive haloes". Astronomy & Astrophysics. 607: A79. doi:10.1051/0004-6361/201731335. ISSN 0004-6361.
- Benavides, José A.; Sales, Laura V.; Abadi, Mario G.; Pillepich, Annalisa; Nelson, Dylan; Marinacci, Federico; Cooper, Michael; Pakmor, Ruediger; Torrey, Paul (2021-09-03), Quiescent Ultra-diffuse galaxies in the field originating from backsplash orbits, arXiv, doi:10.48550/arXiv.2109.01677, arXiv:2109.01677, retrieved 2025-02-03
- "Creating Ultra-Diffuse Galaxies | Center for Astrophysics | Harvard & Smithsonian". www.cfa.harvard.edu. Retrieved 2025-02-03.
Content Disclaimer
Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.
- The information displayed on this website is sourced in part or in whole from Wikipedia and has been adapted for the purpose of restating it. We strive to provide accurate and relevant information, however:
- There is no guarantee of absolute accuracy. Wikipedia is an open, collaborative project that can be edited by anyone, so information is subject to change.
- It is not intended to constitute professional advice. The content displayed is for informational and educational purposes only. For important decisions (e.g., medical, legal, or financial), please consult a professional.
- Content copyright. Wikipedia is licensed under the Creative Commons Attribution-ShareAlike License (CC BY-SA). This means that content may be reused with appropriate attribution and shared under a similar license.
- Responsible use. Any risk arising from the use of information from this website is entirely the responsibility of the user.