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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
Sh_2-1
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 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
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
Emission nebula in Scorpius
around the star Delta Scorpii. It lies next to a large reflection nebula, Sh 2-1. According to the paper Interstellar magnetic cannon targeting the Galactic
Sh_2-7
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
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
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
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
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
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
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
Nebula
Telescope. "Sh 2-294". "Octopus Nebula (Sh 2-294) | Deep⋆Sky Corner". Stromeier, W. (February 2, 1950). "Rote Nebel in der Wintermilchstraβe. Mit 1 Textabbildung"
Sh_2-294
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
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
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
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
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
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
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
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
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
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
Emission nebula
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 cluster Havlen-Moffat 1. However
Sh_2-5
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 2-34, 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
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
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
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
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
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
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
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
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
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 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
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
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
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
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
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
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
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
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
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
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
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
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 2-14 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 2-17 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
The Shavrov Sh-2 (later ASh-2) was a 1930s Soviet amphibious sesquiplane flying boat developed from the Sh-1, with a more powerful engine, slightly increased
Shavrov_Sh-2
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 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
American anti-submarine helicopter
designated HSS-2, which was intended to imply a level of commonality to the earlier HSS-1; it was subsequently redesignated as the SH-3A during the early
Sikorsky_SH-3_Sea_King
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
Supernova remnant
remnant in Cygnus. It is made up of multiple Sharpless Objects. Sh 2-92, Sh 2-94, and Sh 2-96. The nebula was discovered in 1977 during an optical study
SNR_G65.3+5.7
Molecular cloud
Sh 2-24 is a molecular cloud in the constellation Ophiuchus, near the border with Scorpius. It is part of the Sharpless catalog assembled by Stewart Sharpless
Sh_2-24
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
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
Naval helicopter series of the H-60/S-70 family
The Sikorsky SH-60/MH-60 Seahawk (or Sea Hawk) is a twin turboshaft engine, multi-mission United States Navy helicopter based on the United States Army
Sikorsky_SH-60_Seahawk
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
Emission nebula in the Cassiopeia constellation
Sh 2-201 is an emission nebula in the Cassiopeia constellation. It is in the eastern part of the constellation along the eastern border of the IC 1848
Sh_2-201
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
assembled by Stewart Sharpless. It lies next to Sh 2-19. It contains the infrared cluster [DB2000] 1. The nebula appears to be circular in shape. "SIMBAD
Sh_2-18
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
Interstellar cloud in Orion
Northern Sky ASP Monograph Publications, vol. 4, Bo Reipurth, December 2008, p. 757, ISBN 978-1-58381-670-7. CCD Images of the Sharpless Catalog Galaxy Map
Sh_2-264
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
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
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
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 2-309 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
H II region in the constellation Auriga
Sh 2-228 (also known as LBN 784) is an emission nebula and H II region located in the constellation of Auriga. It is part of the Sharpless catalog of 313
Sh_2-228
Instruction set architecture by Hitachi
line, the SH-1 and SH-2, differed only in their support for 64-bit multiplication; the SH-2 supported MUL, DMULS and DMULU, whereas the SH-1 would cause
SuperH
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
Road in New Zealand
State Highway 1 (SH 1) is the longest and most significant road in the New Zealand road network, running the length of both main islands. It appears on
State_Highway_1_(New_Zealand)
Open cluster in the constellation Serpens
solar masses, and a luminosity up to 1 million times that of the Sun. The cluster's age has been estimated to be 1–2 million years. The descriptive names
Eagle_Nebula
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
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
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
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
Camera model
Stylus SH-2 is a digital compact camera announced by Olympus Corporation on March 11, 2015. It differs from its predecessor, the Olympus Stylus SH-1, by
Olympus_Stylus_SH-2
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 Sagittarius
Handbook of Star-Forming Regions: Volume 2 The Southern Sky. Astronomical Society of the Pacific. p. 53. ISBN 978-1-58381-671-4. "Trifid and Lagoon (Image)"
Lagoon_Nebula
1993 series of anti-submarine helicopters
the older Kaman SH-2 Seasprite, which had been serving since the 1960s in a variety of versions. The G model was an evolution of the SH-2F, which was an
Kaman_SH-2G_Super_Seasprite
Supernova remnant in the constellation Taurus
range from about 1–5 M☉, with 2–3 M☉ being the generally accepted value. The neutron star mass is estimated to be between 1.4 and 2 M☉. The predominant
Crab_Nebula
Entry for Saint Helena, Ascension and Tristan da Cunha in ISO 3166-2
ISO 3166-2:SH is the entry for Saint Helena, Ascension and Tristan da Cunha in ISO 3166-2, part of the ISO 3166 standard published by the International
ISO_3166-2:SH
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
Highway in Oklahoma
part of the state, nicknamed Little Dixie. SH-1 is signed east and west. SH-1 eastbound begins at US-177/SH-199 between Mannsville and Madill. It then
Oklahoma_State_Highway_1
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
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
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
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
Road in New Zealand
kilometres, SH 30 is New Zealand's fifth longest provincial (two-digit) state highway, after SH 25, SH 35, SH 73, and SH 94. With the exception of SH 4, it
State Highway 30 (New Zealand)
State_Highway_30_(New_Zealand)
Giant Elliptical galaxy in the constellation Cassiopeia
Maffei, who discovered it and the neighboring Maffei 2 in 1967 via their infrared emissions. Maffei 1 is a slightly flattened core type elliptical galaxy
Maffei_1
Nebula in the constellation Sagitta
1.0 ± 0.5 and C/O = 0.46 ± 0.27. The mass of the nebula's dust has been confirmed to be 0.22 M☉, and the mass of its ionised gas is estimated at 9.2 M☉
M1-67
Galaxy in the constellation Cassiopeia
Maffei 2 is an intermediate spiral galaxy about 10 million light-years away in the constellation Cassiopeia. Maffei 2 and Maffei 1 were both discovered
Maffei_2
Nebula in the constellation Cepheus
application to IC1396". Monthly Notices of the Royal Astronomical Society. 415 (1): 103–32. arXiv:1103.1646. Bibcode:2011MNRAS.415..103B. doi:10.1111/j.1365-2966
Elephant's_Trunk_Nebula
SH 2-1
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SH 2-1
SH 2-1
SH 2-1
SH 2-1
SH 2-1
SH 2-1
SH 2-1