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Helmi stream

From Wikipedia, the free encyclopedia
Stellar stream in the Milky Way Galaxy

TheHelmi Stream is astellar stream of theMilky Way galaxy. It started as a dwarf galaxy, now absorbed by the Milky Way as a stream. It was discovered in 1999, is formed of old stars deficient in heavy elements, and has a mass of 10 to 100 million solar masses. It was absorbed by the Milky Way some 6 to 9 billion years ago.[1]

The stream was named afterAmina Helmi, who discovered this stellar stream after noticing this group of stars all moving at the same speed and in the same direction.[2][3] The Helmi Stream discovery affirmed theories that the merging of galaxies played a significant role in creating the giant structures of the Milky Way galaxy.[2]

In 2024 asubdwarf ofspectral type sdT4 was identified as a possible member of the Helmi stream. Thebrown dwarf is calledCWISE J155349.96+693355.2 has Vtan > 300 km/s and a poorly constrainedradial velocity of +110 ±90 km/s.[4]

Extragalactic planet

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The Helmi stream was briefly believed to be home to the first discoveredplanet purportedly ofextragalactic origin, orbiting the starHIP 13044.[1] However, further analysis of radial velocity data failed to confirm the discovery.[5]

See also

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References

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  1. ^abScientific American,"Extragalactic Expat: Newfound Exoplanet Likely Came from Another Galaxy", John Matson , 18 November 2010
  2. ^ab"Amina Helmi, the "archeologist of the Milky Way," explains how our own galaxy could unlock the mystery of dark matter".FBBVA. 12 December 2017. Retrieved7 November 2019.The idea had already been mooted that the merging of small galaxies could have played a major part in forming today's giant structures. Helmi developed the tools that were able to test this hypothesis and confirm that it held true, at least for the Milky Way.
  3. ^Skibba, Ramin (10 June 2021)."A galactic archaeologist digs into the Milky Way's history".Knowable Magazine.doi:10.1146/knowable-060921-1.S2CID 236290725. Retrieved4 August 2022.
  4. ^Burgasser, Adam J.; Schneider, Adam C.; Meisner, Aaron M.; Caselden, Dan; Hsu, Chih-Chun; Gerasimov, Roman; Aganze, Christian; Softich, Emma; Karpoor, Preethi; Theissen, Christopher A.; Brooks, Hunter; Bickle, Thomas P.; Gagné, Jonathan; Artigau, Étienne; Marsset, Michaël; Rothermich, Austin; Faherty, Jacqueline K.; Kirkpatrick, J. Davy; Kuchner, Marc J.; Andersen, Nikolaj Stevnbak; Beaulieu, Paul; Colin, Guillaume; Gantier, Jean Marc; Gramaize, Leopold; Hamlet, Les; Hinckley, Ken; Kabatnik, Martin; Kiwy, Frank; Martin, David W.; Massat, Diego H.; Pendrill, William; Sainio, Arttu; Schümann, Jörg; Thévenot, Melina; Walla, Jim; Wędracki, Zbigniew; the Backyard Worlds: Planet 9 Collaboration (2 November 2024)."New Cold Subdwarf Discoveries from Backyard Worlds and a Metallicity Classification System for T Subdwarfs".The Astrophysical Journal.982 (2): 79.arXiv:2411.01378.Bibcode:2025ApJ...982...79B.doi:10.3847/1538-4357/adb39f.{{cite journal}}: CS1 maint: numeric names: authors list (link)
  5. ^Jones, M. I.; Jenkins, J. S. (2014). "No evidence of the planet orbiting the extremely metal-poor extragalactic star HIP 13044".Astronomy & Astrophysics.562: id.A129.arXiv:1401.0517.Bibcode:2014A&A...562A.129J.doi:10.1051/0004-6361/201322132.S2CID 55365608.


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