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OB association in the constellation Lacerta
The Lacerta OB1 region is a collection of faint nebular filaments and young, hot stars grouped into an OB association, known as Lacerta OB1; the system
Lacerta_OB1
Emission nebula in Lacerta constellation
approximately 1200 light-years away in the constellation Lacerta. It is a prominent member of the Lacerta OB1 association. The primary source of ionization is
Sh_2-126
Star-forming regions in the constellation Cassiopeia
Cepheus 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
Star-forming regions of Cassiopeia
Star-forming_regions_of_Cassiopeia
X-ray binary system in the constellation Lacerta
700 light years from the Sun. At one time it was considered a member of the Lacerta OB1 association of co-moving stars, but the distance estimate places it well
MWC_656
Nearest OB association to Earth
together several OB associations, including Vela OB2, Orion OB1, Perseus OB2 and Lacerta OB1. With respect to the Sun, the Sco-Cen association coincides
Scorpius–Centaurus association
Scorpius–Centaurus_association
Star in the constellation Lacerta
constellation Lacerta. With an apparent magnitude of 4.9, it is located around 550 parsecs (1,800 ly) distant in the small Lacerta OB1 association. It
10_Lacertae
Star in the constellation Lacerta
red supergiant and a variable star in the constellation Lacerta. It is a member of the Lacerta OB1 stellar association. The MK spectral type of V424 Lac
V424_Lacertae
Star in the constellation Lacerta
doi:10.3390/galaxies13050101. ISSN 2075-4434. Kaltcheva, Nadia (2009). "Lacerta OB1 Revisited". Publications of the Astronomical Society of the Pacific.
2_Lacertae
Star in the constellation Lacerta
Bibcode:1987ApJS...65..581G, doi:10.1086/191237. Kaltcheva, Nadia (October 2009), "Lacerta OB1 Revisited", Publications of the Astronomical Society of the Pacific,
4_Lacertae
Star in the constellation Lacerta
Bibcode:1968ApJS...17..371L, doi:10.1086/190179 Kaltcheva, Nadia (October 2009), "Lacerta OB1 Revisited", Publications of the Astronomical Society of the Pacific,
6_Lacertae
Reflection Nebula in Andromeda
a northeast–southwest orientation. The region is part of the broader Lacerta OB1 star-forming association, several degrees to the west, and is best observed
VdB_158
Binary star in the constellation Lacerta
the constellation Lacerta. Despite being in the constellation of Lacerta, U Lacertae is considered to be a member of the Cepheus OB1 association. It has
U_Lacertae
Star in the constellation Lacerta
doi:10.1086/511002, S2CID 119074863. Kaltcheva, Nadia (October 2009), "Lacerta OB1 Revisited", Publications of the Astronomical Society of the Pacific,
12_Lacertae
American astronomer
Patrick Moore, and Barbara L. Welther), Statistics of the region of Lacerta OB1 (NASA report 1969, with G. V. Coyne and Michele Kaufman), "Advances in
Jaylee_Burley_Mead
Hypergiant star in the constellation Cepheus
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 Gaia
RW_Cephei
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