Cha 110913−773444 (sometimes abbreviated Cha 110913) is an astronomical object surrounded by what appears to be a protoplanetary disk. It lies at a distance...

that such objects be called sub-brown dwarfs. A possible example is Cha 110913−773444, which may either have been ejected and become a rogue planet or formed...

Examples of brown dwarfs surrounded by circumplanetary disks: OTS 44 Cha 110913−773444 WISEA J120037.79-784508.3 2MASS J11151597+1937266 According to van...

planets ejected from their original stellar system (e.g., OTS 44 or Cha 110913−773444), though they are difficult to distinguish from sub-brown dwarfs,...

similarly to stars and are surrounded by protoplanetary disks, such as Cha 110913−773444. As of 2017 there is only one known proto-brown dwarf that is connected...

unambiguously attributed to clouds. CFBDSIR 2149−0403 2MASS J1119–1137 OTS 44 Cha 110913−773444 Jupiter Sanghi, Aniket; Liu, Michael C.; Best, William M.; Dupuy,...

highlighted in December 2005, when the Spitzer Space Telescope observed Cha 110913-773444 (above), only eight times Jupiter's mass with what appears to be the...

called sub-brown dwarfs. Sub-brown dwarfs may be free-floating such as Cha 110913−773444 and OTS 44, or orbiting a larger object such as 2MASS J04414489+2301513...

1845-6357, a binary system comprising a red dwarf and a brown dwarf Cha 110913-773444, an astronomical object that may be a free-floating planet surrounded...

in 2004. On the other hand, the discovery of marginal cases like Cha 110913-773444—a free-floating, planetary-mass object—raises the question of whether...