AI & ChatGPT searches , social queries for SH 2-50
Search references for SH 2-50. Phrases containing SH 2-50
See searches and references containing SH 2-50!
Search references for SH 2-50. Phrases containing SH 2-50
See searches and references containing SH 2-50!SH 2-50
Emission nebula
Sh 2-50 is an emission nebula in Scutum. It is located only 2.5° away from the Eagle Nebula. It is in the direction of the open cluster Dolidze 28. It
Sh_2-50
Sh 2-129 (also known as the Flying Bat Nebula), is a large emission nebula and H II region located in the constellation Cepheus. It is part of the Cepheus
Sh_2-129
Diffuse nebula in Cepheus constellation
Sh 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
Emission nebula in the Cepheus constellation
edu. "Emission Nebula Sh2-140". www.noirlab.edu. Retrieved 2024-09-07. "Sh 2-140". galaxymap.org. Retrieved 2024-09-07. "APOD: 2004 May 20 - Sharpless
Sh_2-140
Molecular cloud
Sh 2-40 is a large nebula in Sagittarius. It is just north of Sh 2-41. Sh 2-40 is in the same direction as powerful radio source W 33. W 33 is, however
Sh_2-40
Emission nebula in Lacerta constellation
Sh 2-126 (also known as Great Lacerta Nebula or Star Funnel Nebula) is a large emission nebula and molecular cloud complex located approximately 1200 light-years
Sh_2-126
Emission nebula
Sh 2-16 is an emission nebula in the constellation Sagittarius. It is ionized by the star LSS 4381. The nebula also contains an infrared cluster, [DB2000]
Sh_2-16
Emission nebula
Sh 2-12 is an emission nebula in Scorpius. It was discovered by Stewart Sharpless in 1951 as he began to work on his catalog of nebulae, which would become
Sh_2-12
Emission nebula or WR* in Canis major
Sh 2-308, also designated as Sharpless 308, RCW 11, or LBN 1052, and commonly known as the Dolphin-Head Nebula, is an H II region located near the center
Sh_2-308
Emission nebula
Sh 2-17 is an emission nebula in the constellation Sagittarius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It contains the infrared
Sh_2-17
Emission nebula in the constellation Orion
Sh 2-279 is an HII region and bright nebulae that includes a reflection nebula located in the constellation Orion. Alternatively, it is designated S279
Sh_2-279
Planetary nebula
Sh 2-68 (also known as Flaming Skull Nebula) is a planetary nebula located in the constellation Serpens. It is the remnant of a low to intermediate mass
Sh_2-68
Emission nebula
Stewart Sharpless. It lies next to the Sharpless objects Sh 2-15, Sh 2-16, Sh 2-17, Sh 2-18, and Sh 2-19. It contains the two infrared clusters, [DB2000] 5
Sh_2-20
Emission nebula
Sh 2-37, also known by the designation IC 1284, or the common name Twiddlebug Nebula, is an emission nebula in the constellation Sagittarius. It is located
Sh_2-37
Planetary nebula in the constellation Cygnus
Sh 2-113 (Sharpless 113) also known as the Flying Dragon Nebula or LBN 333, is a nebula that resembles a supernova remnant (SNR) but with no evidence to
Sh_2-113
Emission nebula
Sh 2-14 is an emission nebula in Scorpius. It is ionized by the supergiant HD 158618 and the giant HD 159090. It is possible Stewart Sharpless initially
Sh_2-14
Emission nebula
Sh 2-44 is a nebula in Sagittarius. It is also known by the designation IC 4701. It is located in the Sagittarius arm of the milky way. NGC 6596 is an
Sh_2-44
Diffuse nebula
Sh 2-48 is a diffuse nebula in Scutum. It is often overlooked due to proximity to the much more famous Eagle Nebula. The open cluster Kronberger 25 is
Sh_2-48
Nebula
Sh 2-185 is an H II region centered on the massive star system Gamma Cassiopeiae (γ Cas) in the northern constellation of Cassiopeia. It was included in
Sh_2-185
Molecular cloud
Sh 2-23 is a molecular cloud in the constellation Scorpius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It is located nearby to
Sh_2-23
Emission nebula
Sh 2-32, also known by the designation IC 1274, is an emission nebula in the constellation Sagittarius. It is a major source of gamma rays. Sh 2-32 was
Sh_2-32
Molecular cloud
Sh 2-307 is a nebula in Puppis. It contains the potential infrared cluster [DBS2003] 8. It is located in the Perseus Arm. Although appearing small visuallly
Sh_2-307
Planetary nebula
Sh 2-78 is a planetary nebula in Aquila. It was discovered by Stewart Sharpless while assembling his catalogue, and identified as a planetary nebula in
Sh_2-78
Nebula in the constellation Serpens
Sh 2-54 is an extended bright nebula in the constellation of Serpens. In its core there are many protostars and many infrared sources; some of these sources
Sh_2-54
Closest planetary nebulae
Sh 2-216 (also known as Sharpless 216) is an ancient planetary nebula located in the constellation Perseus. It is notable for being the closest planetary
Sh_2-216
Emission nebula in Cassiopeia constellation
labels it as a G5 star. The nebula contains a total of 71 variable stars. Sh 2-170 has a magnitude of about 6.5. It is best viewed with a hydrogen-alpha
Sh_2-170
H II region in the constellation Cepheus
Sh 2-155 (also designated Caldwell 9, Sharpless 155 or S155, or LBN529) is a diffuse nebula in the constellation Cepheus, within a larger nebula complex
Sh_2-155
Nebula
Sh 2-294, also known as the Octopus Nebula, is a nebula in Monoceros. It was discovered by Wolfgang Strohmeier in 1950, during a photographic survey. It
Sh_2-294
Nebula
Sharpless 101 (Sh 2-101) is a H II region emission nebula located in the constellation Cygnus. It is sometimes also called the Tulip Nebula because it
Sh_2-101
Molecular Cloud
Sh 2-33 is a molecular cloud in Serpens. It has also been described as a dark globule. It is very faint and has very little color, and must be observed
Sh_2-33
Nebula
Sh 2-1, also known as Sharpless 1, is the combination of a diffuse HII emission nebula and reflection nebula in the constellation of Scorpius with Pi Scorpii
Sh_2-1
Emission nebula
Sh 2-13 is an emission nebula in Scorpius. It is ionized by nearby star HD 158186. Sh 2-13 also contains a star cluster it has formed, Antalova 1. It
Sh_2-13
Emission nebula in constellation Ophiuchus
Sh 2-27 (also known as the Cobold Nebula or the Zeta Ophiuchi Nebula), is an emission nebula in the constellation Ophiuchus. It is ionized by the star
Sh_2-27
Molecular cloud
Sh 2-34, also known as the Forgotten Nebula is a nebula in Sagittarius. It is a star-forming region and contains multiple filamentary structures. Most
Sh_2-34
Emission nebula
Sh 2-19 is an emission nebula in the constellation Sagittarius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It lies next to Sh
Sh_2-19
Emission nebula
Sh 2-38 is a nebula in the constellation Sagittarius. It appears in the shape of a bubble. "SIMBAD query result". Blitz, L.; Fich, M.; Stark, A. A. (1982)
Sh_2-38
H II region
Sh 2-46 (also known as RCW 158), is an H II region, a glowing cloud of ionized hydrogen gas—located in the southern constellation of Serpens. Situated
Sh_2-46
Emission nebula
star's corresponding ring nebula around it are unrelated to Sh 2-22. "Sh 2-22". "Sharpless (Sh2) - Astrobasics". 13 September 2022. "Sh 2-22". v t e
Sh_2-22
Molecular cloud
Sh 2-36 is a molecular cloud in Serpens. It is very faint and requires very dark skies to become visible. "Sh 2-36". "Sharpless (Sh2) - Astrobasics".
Sh_2-36
Emission nebula
Sh 2-15 is an emission nebula in the constellation of Scorpius. It is ionized by the star HD 161853. It is most visible using a Hydrogen-alpha filter.
Sh_2-15
Nebula
Sh 2-10, also called RCW 130, is an emission nebula in the Scorpius constellation. For unknown reasons, it is a significant source of radio emissions.
Sh_2-10
Nebula
Sh 2-112 is a nebula in Cygnus. It is located within the Orion Arm, and is near star complex Cygnus X. It is ionized by the central star BD+45 3216. It
Sh_2-112
Molecular cloud
Sh 2-35 is a nebula in Sagittarius. It is best viewed with a Hydrogen-alpha filter. It is located near to Sh 2-37. combined with Sh 2-37, it has a mass
Sh_2-35
Emission nebula
Sh 2-43 also known as RCW 156, is an emission nebula located in the constellation of Sagittarius. It is a faint, diffuse region of ionized hydrogen gas
Sh_2-43
Nebula
Sh 2-87 is a star-forming nebula with a mass of about 7000 suns. It is close to Sh 2-88, and is located in the central part of the constellation Vulpecula
Sh_2-87
Planetary nebula
Sh 2-42 is a planetary nebula in Sagittarius. It is included in the Sharpless catalogue, however the position indicated by the original catalogue was one
Sh_2-42
Emission nebula
Nebula, listed in the Sharpless catalog as Sh 2-11, and Sh 2-5 itself contains NGC 6337. Like the nearby Sh 2-4, Sh 2-5 is probably ionized by the nearby star
Sh_2-5
Emission nebula in Cygnus constellation
Sh 2-114 (also known as Flying Dragon Nebula) is a faint emission nebula located in the constellation of Cygnus. It lies roughly 4° East-Northeast of star
Sh_2-114
Molecular cloud
Sh 2-47 is a nebula in Serpens. It is probably ionized by the star [L85] S47 3. It is located between Messier 17 and Sh 2-44. "Sh 2-47". "CCD Images of
Sh_2-47
Emission nebula
Sh 2-4 is an emission nebula in the constellation Scorpius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It was originally misidentified
Sh_2-4
HII Region in Scorpius
Sh 2-2, also known as Sharpless 2, is an emission nebula in the constellation of Scorpius. It appears as a mid-range brightness making it difficult to
Sh_2-2
Reflection nebula in the Sagitta constellation
Sh 2-82 (also known as the Little Cocoon Nebula or Little Trifid Nebula) is a small H II region and reflection nebula located in the constellation Sagitta
Sh_2-82
Molecular cloud
Sh 2-41 is a large nebula in Sagittarius and a component of the Small Sagittarius Star Cloud Sh 2-41 appears near the northern edge of the star cloud
Sh_2-41
Emission nebula in the Cassiopeia constellation
light-years away from Earth. It is also seen close to Sh 2-199. It is ionized by infrared cluster [BDB2003] G138.50+01.64. "SH2-201 (IC 1871 )". SharplessCatalog
Sh_2-201
Planetary nebula
Sh 2-71 is a planetary nebula in the constellation of Aquila. It is notable for its highly irregular and complex morphology, which has been attributed
Sh_2-71
Emission nebula in the constellation Cygnus
Sh 2-106, also known as the Celestial Snow Angel, is an emission nebula and a star formation region in the constellation Cygnus. It is a H II region estimated
Sh_2-106
Sh 2-115 is an emission nebula and H II region in the constellation of Cygnus, catalogued by Stewart Sharpless in his 1959 second edition of H II regions
Sh_2-115
HII Region
Sh 2-9, also known as Gum 65, is combination emission and reflection nebula in the Scorpius constellation, surrounding the multiple star system Sigma Scorpii
Sh_2-9
Nebula in the constellation Vulpecula
Sharpless 2-88 or Sh 2-88 is a region including the diffuse nebula Sh 2-88A and the two compact knots Sh 2-88B1 and Sh 2-88B2, all of which are associated
Sh_2-88
Emission nebula in Scorpius
Sh 2-7 is an emission nebula in the Scorpius constellation. The nebula is around the star Delta Scorpii. It lies next to a large reflection nebula, Sh
Sh_2-7
Molecular cloud
Sh 2-312 is a nebula in the southern constellation of Pyxis. It is very large and diffuse, making it largely ignored and unstudied outside of its relation
Sh_2-312
Molecular cloud
Sh 2-309 is a nebula in Puppis. The nebula contains the infrared cluster [DBS2003] 9. It is located beyond the Carina Arm. Sh 2-308 is ionized by the
Sh_2-309
Molecular cloud
only 50 parsecs (~163 light years) away, and the furthest side being 240 parsecs (~783 light years) away. "Sh 2-23". "SH2-24 (Molecular Cloud)". "Sh 2-24"
Sh_2-24
Emission nebula
Sh 2-21 is an emission nebula in the constellation Sagittarius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It is associated with
Sh_2-21
Emission nebula
HD 165921 and HD 166107. Sh 2-31 is located very close to the Lagoon Nebula. Sh 2-31 was discovered, along with nearby Sh 2-29, by John Herschel on 1st
Sh_2-31
Emission nebula
Sh 2-18 is an emission nebula in the constellation Sagittarius. It is part of the Sharpless Catalog assembled by Stewart Sharpless. It lies next to Sh
Sh_2-18
Emission nebula
Sh 2-297 (also known as Sharpless 297) is an emission nebula in the constellation Canis Major. The region was catalogued in 1959 in the extended seconded
Sh_2-297
Interstellar cloud in Orion
Sh 2-1 Sh 2-2 Sh 2-3 Sh 2-4 Sh 2-5 Sh 2-6 Sh 2-7 Sh 2-8 Sh 2-9 Sh 2-10 Sh 2-11 Sh 2-12 Sh 2-13 Sh 2-14 Sh 2-15 Sh 2-16 Sh 2-17 Sh 2-18 Sh 2-19 Sh 2-20
Sh_2-264
Emission nebula and H II region
stars [VM75] Sh 2-305 4 (O8.5V) and [VM75] Sh 2-305 2 (O9.5V) accompanied by a pair of B-type stars [VM75] Sh 2-305 7 (B0V) and [VM75] Sh 2-305 8 (B0V)
Sh_2-305
Molecular cloud in the constellation Canis Major
Sh 2-310 is a nebula in the slightly southern constellation of Canis Major. It is one of the largest H II regions known in the Milky Way. It is ionized
Sh_2-310
Open cluster in the constellation Serpens
million times that of the Sun. The cluster's age has been estimated to be 1–2 million years. The descriptive names reflect impressions of the shape of the
Eagle_Nebula
1959 anti-submarine helicopter family by Kaman
The Kaman SH-2 Seasprite is a ship-based helicopter originally developed and produced by American manufacturer Kaman Aircraft Corporation. It has been
Kaman_SH-2_Seasprite
Emission nebula in Sagittarius
approximately 4,000–6,000 light-years from Earth, the nebula spans 110 by 50 light-years (appearing as 90' by 40' in Earth's sky). While appearing pink
Lagoon_Nebula
Emission nebula
emission nebula in the constellation Sagittarius. RCW 145 contains both Sh 2-26 and Sh 2-28. It is ionized by the supergiant stars LS 4551 and LS 4538. It is
RCW_145
Molecular cloud
Sh 2-306 (also designated RCW 10), is an emission nebula and H II region located in the southern constellation Puppis. It is catalogued in the Sharpless
Sh_2-306
Emission nebula in the constellation Sagittarius
Islands (King Crimson album), which uses an image of the nebula as its cover Sh 2-82, also known as the 'Little Trifid Nebula' NGC 1579, also known as the
Trifid_Nebula
Emission nebula in the constellation Cygnus
temperatures. The Crescent Nebula is a rather small object located about 2 degrees Southwest of Sadr. While considered bright by astronomical imaging
Crescent_Nebula
Nebula
7510. Carsenty, U.; Solf, J. "The kinematical structure of the HII region SH 2-156". "Galactic Nebula IC 1470". Lynds, B.T.; Oniel, E.J., Jr. "An optical
IC_1470
Emission nebula and star cluster in the constellation Vulpecula
NGC 6823 was discovered by William Herschel on July 17, 1785. It is about 50 light-years across and lies about 6,000 light-years away. The center of the
NGC_6820_and_NGC_6823
Nebula located in the constellation of Hydra
Abell 35, also known as Sh 2-313, is a nebula located in the constellation of Hydra, at a distance of 400 light years. The nebula is characterised by its
Abell_35
Open cluster in the constellation Puppis
surrounded by its birth cocoon of gas. The age of H19 is estimated to be 2 Myr, while the age H18 is somewhat controversial, some considering it to be
NGC_2467
Nebula in the constellation Cepheus
The Ghost Nebula (designated Sh 2-136, VdB 141) is a reflection nebula located in the constellation Cepheus. It lies near the cluster NGC 7023. Looking
Ghost_Nebula
Emission nebula in the constellation Cygnus
listed the two nebulae together in his second list of 313 bright nebulae as Sh 2-117. American astronomer Beverly T. Lynds catalogued the obscuring dust cloud
North_America_Nebula
Molecular cloud
"NGC 6857 - HII Ionized region in Cygnus". "Sh 2-99". "Sh 2-100". "Galactic Nebulae NGC 6857 (Sh 2-100) + Sh 2-99". "NOTES FROM OBSERVATION II. NGC 6857"
NGC_6857
Emission nebula in the constellation of Orion
Barnard's Loop (catalogue designation Sh 2-276) is an emission nebula in the constellation of Orion. It is part of the Orion–Eridanus Superbubble, which
Barnard's_Loop
Bipolar planetary nebula in the constellation Scorpius
et al. 2005) Radius = distance × sin(angular size / 2) = 3.4 ± 0.5 kly * sin(>3′.0 / 2) = >1.5 ± 0.2 ly 7.1B apparent magnitude - 5 * (log10(1040 ± 160
NGC_6302
Region of nebulosity in Monoceros constellation
due to its larger presence in the Seagull nebula. The nebula Gum 2, also known as Sh 2-296, forms the Seagull's wings. Seagull Nebula taken by VST OmegaCAM
IC_2177
American anti-submarine helicopter
The Sikorsky SH-3 Sea King (company designation S-61) is an American twin-engine anti-submarine warfare (ASW) helicopter designed and built by Sikorsky
Sikorsky_SH-3_Sea_King
Made of a list
Sh 2-1 Sh 2-2 Sh 2-3 Sh 2-4 Sh 2-5 Sh 2-6 Sh 2-7 Sh 2-8 Sh 2-9 Sh 2-10 Sh 2-11 Sh 2-12 Sh 2-13 Sh 2-14 Sh 2-15 Sh 2-16 Sh 2-17 Sh 2-18 Sh 2-19 Sh 2-20
Sharpless_catalog
Nebula in the constellation Sagitta
Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000-03-01). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30
M1-67
Emission nebula in the constellation Scorpius
them among the more massive stars on record. The young stellar cluster G353.2+0.7 lies east of Pismis 24 and was revealed by a Chandra X-ray image showing
NGC_6357
Emission nebula in the constellation Scorpius
The Astrophysical Journal. 783 (2): 130. arXiv:1401.5377. Bibcode:2014ApJ...783..130R. doi:10.1088/0004-637X/783/2/130. Bakich, Michael E. (2010). 1
NGC_6334
State highway in Twin Falls and Jerome counties in Idaho, United States
State Highway 50 (SH-50) is a 8.092-mile (13.023 km) state highway in Twin Falls and Jerome counties in Idaho, United States, that connects with U.S.
Idaho_State_Highway_50
Open cluster in the constellation Perseus
NGC 1624, also known as Sh 2-212 in the Sharpless catalog, is a very young open cluster in the constellation Perseus inside an emission nebula. It was
NGC_1624
Planetary nebula in the constellation Cygnus
planetary nebula by Heber Doust Curtis in 1919. The central star is magnitude 16.2 Curtis, H.D. "Three New Planetary Nebulae". Steinecke, Wolfgang. "Revised
NGC_6842
Emission nebula
in 1960, whose circular diameter size is 6 arcmin. It also catalogued as Sh 2-3 and Gum 58. Veta S. Avedisova considers RCW 120 is being ionised by the
RCW_120
Nebula in the constellation Cepheus
observations of bright rims in IC 1396". Astronomy and Astrophysics. 75: 345–50. Bibcode:1979A&A....75..345M. Barentsen, G (2011). "T Tauri candidates and
Elephant's_Trunk_Nebula
State highway in Texas
Highway 50 (SH 50) is a 11.679-mile-long (18.796 km) state highway in the northeastern part of the U.S. state of Texas. Its southern terminus is at SH 24 and
Texas_State_Highway_50
Emission nebula in Sagittarius
strongly suggesting the idea of an absorption of the nebulous matter; and, 2. The much feebler and smaller knot at the northwestern end of the same branch
Omega_Nebula
Emission nebula
The Clamshell Nebula (also known as Sh 2-119) is an emission nebula and star-forming region located in the constellation Cygnus. The Clamshell Nebula was
Clamshell_Nebula
SH 2-50
SH 2-50
SH 2-50
SH 2-50
SH 2-50
SH 2-50
SH 2-50
SH 2-50
SH 2-50