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IC 348 information


IC 348
Hubble image of IC 348 and its surroundings.[1]
Observation data (J2000 epoch)
Right ascension03h 44m 34s[2]
Declination+32° 09.8′[2]
Distance1,028 ly (315 pc)[3]
Apparent magnitude (V)7.3[2]
Physical characteristics
Estimated age2 million years
Other designationsC 0341+321, Collinder 41
Associations
ConstellationPerseus
See also: Open cluster, List of open clusters
IC 348 south of Omicron Persei

IC 348 is a star-forming region in the constellation Perseus located about 1,000 light years from the Sun. It consists of nebulosity and an associated 2-million-year-old cluster of roughly 400 stars within an angular diameter of 20″. The most massive stars in the cluster are the binary star system BD+31°643, which has a combined spectral class of B5.[3] Based upon infrared observations using the Spitzer Space Telescope, about half of the stars in the cluster have a circumstellar disk, of which 60% are thick or primordial disks.[4]

  1. ^ "Hubble captures strobe flashes from a young star". ESA/Hubble Press Release. Retrieved 8 February 2013.
  2. ^ a b c Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference apj593_2_1093 was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference aj131_3_1574 was invoked but never defined (see the help page).

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IC 348

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IC 348 is a star-forming region in the constellation Perseus located about 1,000 light years from the Sun. It consists of nebulosity and an associated...

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Tryptophan

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of tryptophan was discovered in the interstellar gas of the star cluster IC 348. Tryptophan is named after the digestive enzymes trypsin, which were used...

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Omicron Persei

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Omicron Persei lies just north of the open cluster IC 348, but is not catalogued as a member. Both IC 348 and Omicron Persei belong to the Perseus OB2 association...

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Dark matter

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to Superplanets: The Low-Mass Initial Mass Function in the Young Cluster IC 348". The Astrophysical Journal. 541 (2): 977–1003. arXiv:astro-ph/0005290....

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Rogue planet

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Cloud Complex, Sigma Orionis cluster, Orion Nebula, Taurus, NGC 1333 and IC 348. A large survey of disks around brown dwarfs and iPMOs with ALMA found that...

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Massive compact halo object

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to Superplanets: The Low-Mass Initial Mass Function in the Young Cluster IC 348*". The Astrophysical Journal. 541 (2): 977–1003. arXiv:astro-ph/0005290...

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LRLL 54361

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flashes, located in the constellation Perseus in the star-forming region IC 348 and 950 light-years away. The object may offer insight into a star's early...

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Perseus molecular cloud

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the Orion molecular cloud it is almost invisible apart from two clusters, IC 348 and NGC 1333, where low-mass stars are formed. It is very bright at mid...

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Barnard 1

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+31° 09′. Barnard 1 contains two reflection nebula regions: NGC 1333 and IC 348 are embedded in the Perseus molecular cloud complex. Hubl, Bernhard (2018-02-24)...

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List of interstellar and circumstellar molecules

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Iglesias-Groth, S. (August 2023). "A search for tryptophan in the gas of the IC 348 star cluster of the Perseus molecular cloud". Monthly Notices of the Royal...

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New General Catalogue

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Catalogues (abbreviated IC), describing a further 5,386 astronomical objects. Thousands of these objects are best known by their NGC or IC numbers, which remain...

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V718 Persei

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star in the constellation of Perseus, located in the young open cluster IC 348. The star has several designations derived from the cluster in which it...

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List of star extremes

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SDSS J091709.55+463821.8 (WD J0917+4638) 2007 0.17 MSun Least massive brown dwarf (unnamed) 2023 3 – 4 MJ Located in the star cluster IC 348 Sub-brown dwarf...

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List of open clusters

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Vela 365 35 14' 4.6 NGC 6633 18h 27.7m +06° 34′ Ophiuchus 375 660 20' 4.6 IC 348 03h 44.6m +32° 10′ Perseus 385 44 7' 7.3 NGC 752 01h 57.7m +37° 47′ Andromeda...

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Hercules A

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radio source in the constellation Hercules corresponding to the galaxy 3C 348. During a survey of bright radio sources in the mid-20th century, astronomers...

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Foundry model

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selling of its own IC-products. The dedicated foundry offers several key advantages to its customers: first, it does not sell finished IC-products into the...

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Collinder catalogue

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426 are asterisms. Cr 32, 33, and 34 all refer to parts of the much larger IC 1848. There is some doubt as to whether or not Cr 84, 182, 221, 254, 265,...

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Walgreens

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Economy: Concepts and Cases, Second Edition. Boca Raton, FL: CRC Press. p. 348. ISBN 0-203-50149-7. Ried, Adam (2012). Thoroughly Modern Milkshakes: 100...

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Beat Bobby Flay

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Rita Jammet, Michael Jenkins Kati roll Avishar Barua 412 16 "Bouillabaisse-ic Instinct" May 18, 2023 (2023-05-18) Jet Tila, Sunny Anderson Great Northern...

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Diisobutyl phthalate

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Metra Electric District

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orange" to reflect the line's origins with the Illinois Central Railroad (IC) and its Panama Limited passenger train. Apart from the spots where its tracks...

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structural heart disease or ischemic heart disease. Flecainide is a class Ic antiarrhythmic agent. It works by decreasing the entry of sodium in heart...

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Phases of ice

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−211 °C (62 K; −348 °F); below that temperature, the ice expands again (negative thermal expansion). Besides ice Ih, a small amount of ice Ic may occasionally...

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Illinois Central 2613

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coal; a design feature that was rare on IC steam locomotives. The 2600 class was a step-up design of the IC 2500 class 4-8-2's, and their design was...

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Marxists-Leninists members. In 1994, its press organ named Intervention Communiste (IC) was launched. At the faction's 4th national conference, a minority group...

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