Iscandar Cluster: Difference between revisions
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*[[Wol system|Wol]] | *[[Wol system|Wol]] | ||
*[[Wolf system|Wolf]] | *[[Wolf system|Wolf]] | ||
*[[Yabu system|Yabu]] | |||
*[[Yamamoto system|Yamamoto]] | *[[Yamamoto system|Yamamoto]] | ||
*[[Yamanami system|Yamanami]] | *[[Yamanami system|Yamanami]] | ||
*[[Yamazaki system|Yamazaki]] | *[[Yamazaki system|Yamazaki]] | ||
*[[Yuki system|Yuki]] | *[[Yuki system|Yuki]] | ||
*[[Yurisha system|Yurisha]] | *[[Yurisha system|Yurisha]] | ||
Revision as of 20:27, 24 February 2023
The Iscandar Cluster is a large group of star systems in the Celestial Lance Universe that are relatively close to each other in real space and connected via wormholes.
The star systems in the cluster include:
- Ageha
- Akagi
- Alphon
- Ankoku
- Arakome
- AU-09
- Balcom
- Barreled
- Bemlayze
- Berger
- Bolar
- Dagon
- Daslugens
- Desler
- Destar
- Dingir
- Ditz
- Domel
- Domon
- Etos
- Fraken
- Frauski
- Ganz
- Garmilas
- Gatlantis
- Gehlen
- Geidel
- Garemund
- Getto
- Göru
- Grotus
- Gustav
- Hayashi
- Heidern
- Heigel
- Heiji
- Helmeyer
- Herm
- Hirata
- Hiss
- Histenberger
- Iliya
- Iscandar
- Kaoru
- Kazan
- Keeling
- Kitano
- Kodai
- Kreuz
- Levars
- Lugal
- Mazor
- Meisernomdrum
- Metzler
- Miezela
- Miikun
- Miru
- Mölders
- Namio
- Nanbu
- Nazca
- Nemoto
- Okita
- Ōta
- Paren
- Pascal
- Raiden
- Ram
- Ryuu
- Sabera
- Saburo
- Sada
- Saitō
- Sakezo
- Saleluya
- Sasha
- Schultz
- Seafrage
- Serizawa
- Shima
- Shiro
- Starsha
- Sugiyama
- Sukaru
- Susumu
- Talan
- Teresa
- Tōdō
- Tokugawa
- Valus
- Vandevere
- Wol
- Wolf
- Yabu
- Yamamoto
- Yamanami
- Yamazaki
- Yuki
- Yurisha