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OB Association in the constellation Cepheus
Cepheus OB1 is an OB association around the cluster NGC 7380. The region is approximately 3,400 parsecs from Earth in the constellation of Cepheus, although
Cepheus_OB1
Group of OB stars
of Orion Molecular Cloud Complex. Image of Cepheus OB3 OB stars Cepheus OB2 Region Cepheus OB3 Region Cepheus OB4 Region Stellar associations Sagittarius
OB_association
Diffuse nebula in Cepheus constellation
2-132, also known as the Lion Nebula, is a diffuse nebula in Cepheus. It is part of the Cep OB1 Association and located in the Perseus Arm of the galaxy.
Sh_2-132
OB association in the constellation Scorpius
The Scorpius OB1 region is a large nebular region of the Milky Way located on the Sagittarius Arm in the direction of the constellation Scorpius, where
Scorpius_OB1
nebular complexes, but south of the Cepheus line of sight, there is a rather sparse OB association known as Lacerta OB1; at a distance of 2600 light-years
Star-forming regions of Cassiopeia
Star-forming_regions_of_Cassiopeia
Dark nebula in the constellation Camelopardalis
young stellar objects and the OB association catalogued as Camelopardalis OB1, composed of some bright stars of spectral class O and B, plus several dozen
Camelopardalis_dark_region
Black Hole in the constellation Cepheus
blazar, located near the high declination region of the constellation Cepheus, near the North Equatorial Pole. The object is an OVV (optically violent
S5_0014+81
Stars sorted by absolute magnitude
of the molecular cloud G291.27-0.71. IC 4996 is an open cluster in Cygnus OB1. Vela R2 is a OB association in Vela Molecular Ridge. Lists of astronomical
List_of_most_luminous_stars
WD 0145+234 (star disrupting an exoasteroid) Assuming membership to Cepheus OB1 ASASSN-21js's temperature of 14800+4200 −2800 K lies within the temperature
List of stars that have unusual dimming periods
List_of_stars_that_have_unusual_dimming_periods
Star in the constellation Cepheus
Iota Cephei is a star in the northern constellation Cepheus. Its name is a Bayer designation that is Latinized from ι Cephei, and abbreviated Iota Cep
Iota_Cephei
Hypergiant star in the constellation Cepheus
its spectroscopic luminosity and it is assumed to be a member of the Cepheus OB1 association, placing it within the Perseus Arm of the Milky Way. The
RW_Cephei
Star in the constellation Cepheus
Cephei is a white-hued binary star system in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from θ Cephei, and abbreviated
Theta_Cephei
Coherent, wave-shaped gaseous structure in the Milky Way
and has further large star-forming regions such as Monoceros OB1, California Nebula, Cepheus Far, and Rho Ophiuchi. A 2024 paper announced the discovery
Radcliffe_wave
Star in the constellation Cepheus
a different unique acronym for V354 Cephei. V354 Cephei is near the Cepheus OB1 stellar association and considered a likely member, although the star
V354_Cephei
Variable star in the constellation Cepheus
binary and variable star located in the constellation Cepheus. It is thought to be a member of the Cep OB1 stellar association at about 8,000 light years. W
W_Cephei
Globular cluster in the constellation Cepheus
is a globular cluster, part of the Palomar group in the constellation Cepheus in the halo possibly in the Outer Arm of the Milky Way galaxy. First discovered
Palomar_1
Star in the constellation Cepheus
Epsilon Cephei is a star in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ε Cephei, and abbreviated Epsilon
Epsilon_Cephei
Star in the constellation Cepheus
Rho2 Cephei is a solitary star in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ρ2 Cephei, or simply ρ
Rho2_Cephei
Star in the constellation Cepheus
Rho1 Cephei is a double star located in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ρ1 Cephei, and abbreviated
Rho1_Cephei
Nebula in the constellation Cepheus
SSTGFLS J222557+601148 is a planetary nebula in the constellation Cepheus. Located between 2000 and 3000 parsecs distant from Earth, it was originally
SSTGFLS_J222557+601148
Star cluster in the Cepheus constellation
NGC 7055 is an open cluster located in the Cepheus constellation. It was discovered by 19th century English astronomer John Herschel on 25 September 1829
NGC_7055
Binary star in the constellation Lacerta
constellation of Lacerta, U Lacertae is considered to be a member of the Cepheus OB1 association. It has been listed as a member of the open cluster ASCC
U_Lacertae
Dark nebula in the constellation Cepheus
L 1157 is a dark nebula in the constellation Cepheus. It was catalogued in 1962 by U.S. astronomer Beverly T. Lynds in her Catalogue of Dark Nebulae,
L1157
Giant molecular cloud in the Milky Way
brilliant OB associations: This is the case with the "southernmost" Cygnus OB1 association, Cygnus OB9, and especially the very bright Cygnus OB2, which
Cygnus Molecular Nebula Complex
Cygnus_Molecular_Nebula_Complex
discoverer. It was previously believed that IC 4996 was a member of the Cyg OB1 stellar association, however the cluster is located 4.6 times further away
IC_4996
Stellar classification
stellar and substellar candidate companions around massive stars in Sco OB1 and M17". The Astronomical Journal. 168 (5): 209. arXiv:2409.16212. Bibcode:2024AJ
O-type_star
Open cluster in the constellation Cygnus
local arm). According to the Sky Catalogue, M29 is included in the Cygnus OB1 association, and the radial velocity component of three-dimensional motion
Messier_29
Planetary nebula in the constellation Camelopardalis
Uppsala General Catalogue, as UGC 7731. NGC 40 (the Bow-Tie Nebula in Cepheus) Cragin, Murray; Lucyk, James; Rappaport, Barry (1993). The Deep-sky Field
Lemon_Slice_Nebula
II region in Small Magellanic Cloud. IC 4996 is an open cluster in Cygnus OB1. Vela R2 is a OB association in Vela Molecular Ridge. Black holes are the
List_of_most_massive_stars
Star in the constellation Cygnus
5Ia in the constellation Cygnus. It is considered a member of the Cygnus OB1 stellar association, and within it the open cluster Berkeley 87, which would
BC_Cygni
Star in the constellation Cygnus
and a minimum of magnitude 9.9. It is considered a member of the Cygnus OB1 stellar association, its distance is around 1,300 parsecs (4,200 ly) of the
BI_Cygni
Cluster of massive and luminous stars
P.; Palmer, J.; Cleeves, L.I. (2012). "Irradiated interfaces in the Ara OB1, Carina, Eagle Nebula, and Cyg OB2 massive star formation regions". High
Cygnus_OB2
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