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Group of stars
Camelopardalis OB1 (Cam OB1) is a group of young stars that share a common origin and a similar motion through space, but, as a whole, are no longer gravitationally
Camelopardalis_OB1
Dark nebula in the constellation Camelopardalis
number of young stellar objects and the OB association catalogued as Camelopardalis OB1, composed of some bright stars of spectral class O and B, plus several
Camelopardalis_dark_region
Double star system in the constellation Camelopardalis
conditions. The 1 Camelopardalis system is part of the Camelopardalis OB1 stellar association, which is 820 pc away. 1 Camelopardalis A is a hot massive
1_Camelopardalis
Binary star in the constellation Camelopardalis
CS Camelopardalis (CS Cam; HD 21291) is a binary star in reflection nebula VdB 14, in the constellation Camelopardalis. It is a 4th magnitude star, and
CS_Camelopardalis
Group of OB stars
Retrieved 2026-06-19. "Ass Cen OB1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2026-06-19. "Ass Cep OB1". SIMBAD. Centre de données
OB_association
Star in the constellation Camelopardalis
reflection nebula VdB 15, in the constellation Camelopardalis. It has the variable star designation CE Camelopardalis, abbreviated CE Cam. It is a magnitude 4
HD_21389
Star in the constellation Camelopardalis
Gamma Camelopardalis, also named Shaowei, is a suspected wide binary star system in the northern circumpolar constellation of Camelopardalis. Its name
Gamma_Camelopardalis
Galaxy cluster in the constellation Camelopardalis
MS 0735.6+7421 is a galaxy cluster located in the constellation Camelopardalis, approximately 2.6 billion light-years away. It is notable as the location
MS_0735.6+7421
Loose star cluster
doi:10.1086/111771. Lyder, David A. (November 2001). "The Stars in Camelopardalis OB1: Their Distance and Evolutionary History". The Astronomical Journal
Stellar_association
July 2004 supernova event in the constellation Camelopardalis
a star in a young, compact star cluster in the galaxy NGC 2403, in Camelopardalis. The cluster had been cataloged as the 96th object in a list of luminous
SN_2004dj
One of the farthest known galaxies from the Earth in the constellation Camelopardalis
Space Telescope. The location of the galaxy is in the constellation Camelopardalis, which is also the location of the gravitational lensing cluster that
MACS0647-JD
Binary star in the constellation Camelopardalis
Struve 1694 (Σ 1694, Struve 1694) is a double star in the constellation Camelopardalis. Σ 1694 is a double star, with components of magnitudes 5.3m and 5.9m:
Struve_1694
Planetary nebula in the constellation Camelopardalis
is 1.3 kiloparsecs (4500 ly) away from Earth in the constellation of Camelopardalis (just 7.5 degrees from Polaris). It is a relatively young nebula and
Lemon_Slice_Nebula
Supernova in the constellation Camelopardalis
SN 2010lt is a supernova located in the galaxy UGC 3378 in Camelopardalis. It was discovered by amateur astronomers Kathryn Aurora Gray, her father Paul
SN_2010lt
Galaxy cluster in the constellation Camelopardalis
lies between the Big Dipper and Little Dipper in the constellation Camelopardalis. It is part of a sample of 12 extreme galaxy clusters at z > 0.5 discovered
MACS_J0647.7+7015
Open cluster in the constellation Camelopardalis
a young open cluster of approximately 60 stars in the constellation Camelopardalis, discovered by William Herschel on November 3, 1787. It has a visual
NGC_1502
Star-forming regions in the constellation Cassiopeia
line of sight, there is a rather sparse OB association known as Lacerta OB1; at a distance of 2600 light-years (800 parsecs), one of the largest giant
Star-forming regions of Cassiopeia
Star-forming_regions_of_Cassiopeia
Small open cluster in the constellation Perseus
Σ446, with a magnitude 6.7 primary. The cluster is a member of the Camelopardalis OB1 association. Kharchenko, N. V.; et al. (2013). "Global survey of star
NGC_1444
Pattern of stars recognized on Earth's night sky
group of stars, but the stars of Orion's Belt are all members of the Orion OB1 association and five of the seven stars of the Big Dipper are members of
Asterism_(astronomy)
Stars sorted by absolute magnitude
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. Lists of astronomical
List_of_most_luminous_stars
Hot, luminous star with a spectral type of A9 or earlier
"High-resolution spectroscopic study of massive blue and red supergiants in Perseus OB1 - I. Definition of the sample, membership, and kinematics". Astronomy & Astrophysics
Blue_supergiant
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
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
(April 2014). "CHARA/MIRC Observations of Two M Supergiants in Perseus OB1: Temperature, Bayesian Modeling, and Compressed Sensing Imaging". The Astrophysical
List_of_largest_stars
Astronomical object emitting X-rays
interior is energized by UV light and stellar winds from hot stars in the Orion OB1 association. These stars energize a superbubble about 1200 lys across which
Astrophysical_X-ray_source
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