NGC 7635, also known as the Bubble Nebula, Sharpless 162, or Caldwell 11, is an H II region emission nebula in the constellation Cassiopeia. It lies close to the open cluster Messier 52. The "bubble" is created by the stellar wind from a massive hot, 8.7 magnitude young central star, SAO 20575 (BD+60°2522). The nebula is near a giant molecular cloud which contains the expansion of the bubble nebula while itself being excited by the hot central star, causing it to glow. It was discovered in November 1787 by William Herschel. The star BD+60°2522 is thought to have a mass of about 44 M☉.
NGC 70 is a spiral galaxy located in the constellation Andromeda. It was discovered on October 7, 1855, by R. J. Mitchell and was also observed on December 19, 1897 by Guillaume Bigourdan from France who described it as "extremely faint, very small, round, between 2 faint stars".
NGC 276 is a barred spiral galaxy located approximately 626 million light-years from the Solar System in the constellation Cetus. It was discovered in 1886 by Frank Muller and was later also observed by DeLisle Stewart.
NGC 331 is a barred spiral galaxy in the constellation Cetus. It was discovered in 1886 by Francis Leavenworth. It was described by Dreyer as "extremely faint, very small, round, a little brighter middle, 12th magnitude star 3 arcmin northeast." There are two candidates as to which object is NGC 331: PGC 2759 or PGC 3406, with the former being a much more likely candidate than the latter.
NGC 343 are a pair of interacting galaxies in the constellation Cetus. It was discovered in 1886 by Frank Muller. It was described by Dreyer as "extremely faint, very small, irregularly round, suddenly brighter middle and nucleus ."
NGC 344 is a barred spiral galaxy in the constellation Cetus. It was discovered in 1886 by Frank Muller. It was described by John Louis Emil Dreyer as "extremely faint, very small, irregularly round, suddenly brighter middle and nucleus ."
NGC 348 is a spiral galaxy in the constellation Phoenix. It was discovered on October 3, 1834 by John Herschel. It was described by Dreyer as "extremely faint, small, round."
NGC 350 is a lenticular galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It was described by Dreyer as "extremely faint."
NGC 351 is a spiral galaxy in the constellation Cetus. It was discovered on November 10, 1885 by Lewis Swift. It was described by Dreyer as "extremely faint, pretty small, northwestern of 2.", the other being NGC 353.
NGC 353 is a spiral galaxy in the constellation Cetus. It was discovered on November 10, 1885 by Lewis Swift. It was described by Dreyer as "extremely faint, pretty small, round, southeastern of 2.", the other being NGC 351.
NGC 355 is a lenticular galaxy in the constellation Cetus. It was discovered on September 27, 1864 by Albert Marth. It was described by Dreyer as "extremely faint, very small."
NGC 359 is an elliptical galaxy located approximately 238 million light-years from the Solar System in the constellation Cetus. It was discovered on September 2, 1864, by Albert Marth. It was described by Dreyer as "extremely faint, very small."
NGC 360 is a spiral galaxy located approximately 103 million light-years from the Solar System in the constellation Tucana. It was discovered on 2 November 1834 by John Herschel. Dreyer, creator of the New General Catalogue described the object as "extremely faint, very much extended 145°, very little brighter middle."
NGC 389 is a lenticular galaxy located approximately 239 million light-years from the Solar System in the constellation Andromeda. It was discovered on September 6, 1885 by Lewis Swift. It was described by Dreyer as "extremely faint, extremely small, round, star near."
NGC 397 is a lenticular galaxy located in the constellation Pisces. It was discovered on December 6, 1866, by Robert Ball. It was described by Dreyer as "extremely faint, small, round, very faint star to west."
NGC 409 is an elliptical galaxy located in the constellation Sculptor. It was discovered on November 29, 1837 by John Herschel. It was described by Dreyer as "extremely faint, small, round, very small (faint) star near."
NGC 413 is a spiral galaxy of type SB(r)c located in the constellation Cetus. It was discovered in 1886 by Francis Leavenworth. It was described by Dreyer as "extremely faint, pretty small, very little extended."
NGC 417 is a lenticular galaxy of type SAB0− located in the constellation Cetus. It was discovered in 1886 by Francis Leavenworth. It was described by Dreyer as "extremely faint, extremely small, round."
NGC 423 is a lenticular galaxy of type S0/a? located in the constellation Sculptor. It was discovered on November 14, 1835 by John Herschel. It was described by Dreyer as "extremely faint, small, extended, gradually a little brighter middle, eastern of 2.", the other being NGC 418.
NGC 5502 is a spiral galaxy in the constellation of Ursa Major, registered in New General Catalogue (NGC).
