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Longer titles found: List of nearby stellar associations and moving groups (view)

searching for Stellar association 29 found (124 total)

LH 95 (341 words) [view diff] exact match in snippet view article find links to article

of LH 95. Previously only young bright stars were known in this stellar association. Imaging using the Hubble Space Telescope, however, allowed the identification

Vulpecula (1,392 words) [view diff] no match in snippet view article find links to article

Vulpecula /vʌlˈpɛkjʊlə/ is a faint constellation in the northern sky. Its name is Latin for "little fox", although it is commonly known simply as the fox

NGC 2404 (288 words) [view diff] exact match in snippet view article find links to article

is probably much less compact, so it probably looks like a large stellar association. This H II region is probably only a few million years old. "NASA/IPAC

Orion–Eridanus Superbubble (149 words) [view diff] exact match in snippet view article find links to article

overlapping supernova remnants that may be associated with the Orion OB1 stellar association; the bubble is approximately 1200 ly across. It is the nearest superbubble

NGC 1313 (799 words) [view diff] exact match in snippet view article find links to article

-4) This means that the WO is likely part of a binary or a small stellar association. Two supernovae have been observed in NGC 2841: SN 1962M (type II

CK Carinae (651 words) [view diff] exact match in snippet view article find links to article

around 2,300 pc, and is thought to be a member of the Carina OB1-D stellar association which is at a distance of about 2,200 pc. An analysis of the distances

Trumpler 14 (912 words) [view diff] exact match in snippet view article find links to article

nearby Trumpler 16, they are the main clusters of the Carina OB1 stellar association, which is the largest association in the Carina Nebula, although

HD 206267 (463 words) [view diff] exact match in snippet view article find links to article

protoplanetary disks. The system is a member of the Cepheus OB2 stellar association, which notably includes evolved blue and red supergiants such as

HD 93129 (1,195 words) [view diff] exact match in snippet view article find links to article

Trumpler 14 star cluster, a young star cluster within the Carina OB1 stellar association that harbors other super-luminous stars, like Eta Carinae and WR

Collinder catalogue (535 words) [view diff] exact match in snippet view article find links to article

11 globular clusters, 6 asterisms, 1 stellar moving group, and 1 stellar association. Catalogue objects are denoted by Collinder, e.g. "Collinder 399"

Eta Muscae (677 words) [view diff] exact match in snippet view article find links to article

It is a member of the Lower Centaurs Crux subgroup of the Sco OB2 stellar association of co-moving stars. The two main components of this system form a

Carina Nebula (3,723 words) [view diff] exact match in snippet view article find links to article

500 pc) from Earth. It is one of the main clusters of the Carina OB1 stellar association, which is the largest association in the Carina Nebula. About 2,000

NGC 602 (827 words) [view diff] case mismatch in snippet view article find links to article

R., et al., 2007 ApJL 665, 109 "The Initial Mass Function of the Stellar Association NGC 602 in the Small Magellanic Cloud with Hubble Space Telescope

Trumpler 16 (1,236 words) [view diff] exact match in snippet view article find links to article

Trumpler 14 are the most prominent star clusters in Carina OB1, a giant stellar association in the Carina spiral arm. Another cluster within Carina OB1, Collinder

DS Tucanae (1,417 words) [view diff] case mismatch in snippet view article find links to article

Zuckerman, B.; Webb, R. A. (2000-06-01). "Identification of a Nearby Stellar Association in theHipparcos Catalog: Implications for Recent, Local Star Formation"

HD 106906 b (1,870 words) [view diff] exact match in snippet view article find links to article

found a C/O=0.53+0.15 −0.25 for HD 106906 b, consistent with the stellar association its host star formed in. This is consistent with stellar-like formation

Vela (constellation) (2,552 words) [view diff] exact match in snippet view article

Naylor, T.; Walter, F. M.; Pozzo, M. P.; Devey, C. R. (2009). "The stellar association around Gamma Velorum and its relationship with Vela OB2". Monthly

Gamma Velorum (1,516 words) [view diff] exact match in snippet view article find links to article

Naylor, T.; Walter, F. M.; Pozzo, M. P.; Devey, C. R. (2009). "The stellar association around Gamma Velorum and its relationship with Vela OB2". Monthly

Stephenson 2 DFK 1 (2,423 words) [view diff] exact match in snippet view article find links to article

casting doubt on its membership. As stated in a 2012 study, the stellar association is spread over a large area, with Stephenson 2 blending into its

Zeta Puppis (1,995 words) [view diff] exact match in snippet view article find links to article

suggestions for the birthplace of Zeta Puppis were the very young Vela R2 stellar association at around 800pc and the Vela OB2 association at 450pc. Neither origin

Melotte 186 (553 words) [view diff] exact match in snippet view article find links to article

existence; on the other hand, Mel 186 can also be seen as a scattered stellar association rather than a real open cluster due to the considerable distance

S Doradus (3,188 words) [view diff] exact match in snippet view article find links to article

brightest member of the open cluster NGC 1910, also known as the LH41 stellar association, visible in binoculars as a bright condensation within the main bar

Vega (10,142 words) [view diff] exact match in snippet view article find links to article

Based on this star's kinematic properties, it appears to belong to a stellar association called the Castor Moving Group. However, Vega may be much older than

ʻOumuamua (10,757 words) [view diff] case mismatch in snippet view article find links to article

(2017). "Origin of Interstellar Object A/2017 U1 in a Nearby Young Stellar Association?". Research Notes of the AAS. 1 (1): 13. arXiv:1711.01300. Bibcode:2017RNAAS

Adrian Price-Whelan (289 words) [view diff] case mismatch in snippet view article find links to article

Semyeong; Evans, N. Wyn (December 16, 2019). "Spectroscopy of the Young Stellar Association Price-Whelan 1: Origin in the Magellanic Leading Arm and Constraints

List of most massive stars (8,888 words) [view diff] exact match in snippet view article find links to article

DEM S80 is a H II region in Small Magellanic Cloud. GKK-A144 is a stellar association in Large Magellanic Cloud. BSDL 2242 is a star cluster in Large Magellanic

ST Cephei (346 words) [view diff] exact match in snippet view article find links to article

by the Hipparcos satellite. Its membership in the Cepheus OB2-B stellar association allows its distance to be estimated at 830 parsecs, or 2,715 light

NGC 2001 (164 words) [view diff] exact match in snippet view article find links to article

light years across. NGC 2001 is also listed as part of Lucke-Hodge stellar association 64, along with ANONb4 and e135. "NGC 2001". SIMBAD. Centre de données

Gliese 900 (1,571 words) [view diff] exact match in snippet view article find links to article

of being a field star, i.e. not associated to any star cluster or stellar association. A 2024 study led by Austin Rothermich identified CWISE J233531.55+014219