Galactic Center filament

An MeerKAT image of the Galactic Center showing a number of filaments
Radio image of a number of parallel filaments in the Galactic Center; Sagittarius A*, the Milky Way's central black hole, is located in the bright region in the bottom right[1][2]
Nonthermal radio filaments from the 4'' resolution MeerKAT mosaic; oriented vertically for space; scales given assuming a distance of 8.2 kpc

Galactic Center filaments are large radio-emitting[3] filament-shaped structures found in the Galactic Center of the Milky Way.[4] Their cause is unknown.[4] Both vertical and horizontal filaments exist, running vertically (perpendicular to the galactic plane) and horizontally (parallel to the galactic plane) away from the Galactic Center, respectively.[4][5] Vertical filaments possess strong magnetic fields[6] and emit synchrotron radiation: radiation emitted by particles moved at near-lightspeed through a magnetic field.[4] Although theories have been proposed, the source of these particles is unknown.[4][7] Horizontal filaments appear to emit thermal radiation, accelerating thermal material in a molecular cloud.[3] They have been proposed to be caused by the outflow from Sagitarius A*, the Milky Way's central black hole, impacting vertical filaments and H II regions of ionized gas around hot stars.[4]

While the vertical filaments can reach 150 light years in length, the horizontal filaments are much shorter, usually around 5 to 10 light years long.[5] A few hundred horizontal filaments exist (figure given as of 2023), far fewer than the number of vertical filaments.[5] Vertical filaments were discovered in 1984 by Farhad Yusef-Zadeh, Mark Morris, and Don Chance;[citation needed] horizontal filaments were discovered in 2023 by Yusef-Zadeh, Ian Heywood and collaborators.[4]

Vertical filaments are often found in pairs and clusters, often stacked equally spaced side by side similar to the strings of a harp.[6] As of 2022, it was unknown why they formed in clusters or in a regularly spaced manner.[7]

History

[edit]

Galactic Center filaments, specifically vertical filaments,[4] were first discovered in a 1984 publication by Yusef-Zadeh et al..[8][9] They were discovered unexpectedly, and initially considered to be possible artifacts, but confirmed after being observed at multiple wavelengths by multiple groups.[4]

Because the earliest filaments detected were all vertical filaments, oriented perpendicular to the galactic plane, early theories suggested that they may have been related to the Milky Way's magnetic field, oriented in the same manner.[10] A number of theories had been proposed by 1996.[11] One proposal at the time suggested the filaments were cosmic strings.[11] This faced several difficulties, including that the lack of observed oscillation of the strings, and the apparent splitting of some of the filaments.[11]

Subsequently, before 2004, weaker filaments were discovered not perpendicular to the galactic plane.[10] These were initially believed to be oriented randomly in respect to it, and at the time presented difficulties for hypotheses relating Galactic Center filaments to the galactic magnetic field.[10] The radiation emitted from vertical filaments is now known to be synchrotron radiation, caused by particles moving at nearly the speed of light through a magnetic field.[4]

A detailed radio image of the Galactic Center by the MeerKAT telescope published in February 2022[2] led to the discovery of about ten times more filaments than had been previously known, allowing researchers to study the filaments statistically.[6] Horizontal filaments were discovered in a June 2023 publication by Yusef-Zadeh et al..[4][12] According to Yusef-Zadeh, they were identified by statistical tests after he happened to notice, looking at images of the filaments, that many seemed to be pointing radially away from the Galactic Center.[4]

References

[edit]
  1. ^ Cimone, Matthew (2022-02-21). "Imaging the Galaxy's Centre in Unprecedented Detail Reveals More Mysterious Filaments". Universe Today. Retrieved 2024-09-07.
  2. ^ a b Heywood, I.; Rammala, I.; Camilo, F.; Cotton, W. D.; Yusef-Zadeh, F.; Abbott, T. D.; Adam, R. M.; Adams, G.; Aldera, M. A.; Asad, K. M. B.; Bauermeister, E. F.; Bennett, T. G. H.; Bester, H. L.; Bode, W. A.; Botha, D. H. (2022-02-01). "The 1.28 GHz MeerKAT Galactic Center Mosaic". The Astrophysical Journal. 925 (2): 165. arXiv:2201.10541. Bibcode:2022ApJ...925..165H. doi:10.3847/1538-4357/ac449a. ISSN 0004-637X.
  3. ^ a b "Mysterious dashes revealed in Milky Way's center". ScienceDaily. Retrieved 2024-09-07.
  4. ^ a b c d e f g h i j k l Bartels, Meghan. "Strange Giant Filaments Reveal a Mystery at the Milky Way's Heart". Scientific American. Retrieved 2024-09-06.
  5. ^ a b c "Hundreds of Strange Filaments Surround the Galactic Center". Discover Magazine. Retrieved 2024-09-07.
  6. ^ a b c Choi, Charles Q. (2022-02-01). "New Milky Way mosaic reveals nearly 1,000 strange 'filaments' at the heart of our galaxy". Space.com. Retrieved 2024-09-07.
  7. ^ a b Specktor, Brandon (2022-01-29). "Astronomers discover 1,000 strange 'filaments' of radio energy bursting from the galaxy's center". LiveScience. Retrieved 2024-09-07.
  8. ^ Yusef-Zadeh, F.; Arendt, R. G.; Wardle, M.; Heywood, I. (June 2023). "The Population of the Galactic Center Filaments: Position Angle Distribution Reveals a Degree-scale Collimated Outflow from Sgr A* along the Galactic Plane". The Astrophysical Journal Letters. 949 (2): L31. arXiv:2306.01071. Bibcode:2023ApJ...949L..31Y. doi:10.3847/2041-8213/acd54b. ISSN 2041-8205.
  9. ^ Yusef-Zadeh, F.; Morris, Mark; Chance, D. (August 1984). "Large, highly organized radio structures near the galactic centre". Nature. 310 (5978): 557–561. Bibcode:1984Natur.310..557Y. doi:10.1038/310557a0. ISSN 1476-4687.
  10. ^ a b c "Origin of Enigmatic Galactic-center Filaments Revealed". National Radio Astronomy Observatory. Retrieved 2024-09-23.
  11. ^ a b c Morris, Mark (1996), Blitz, Leo; Teuben, Peter (eds.), "What are the Radio Filaments Near the Galactic Center?", Unsolved Problems of the Milky Way: Proceedings of the 169th Symposium of the International Astronomical Union, held in the Hague, the Netherlands, August 23–29, 1994, Dordrecht: Springer Netherlands, pp. 247–261, doi:10.1007/978-94-009-1687-6_31, ISBN 978-94-009-1687-6, retrieved 2024-09-23
  12. ^ Yusef-Zadeh, F.; Arendt, R. G.; Wardle, M.; Heywood, I. (2023-06-01). "The Population of the Galactic Center Filaments: Position Angle Distribution Reveals a Degree-scale Collimated Outflow from Sgr A* along the Galactic Plane". The Astrophysical Journal Letters. 949 (2): L31. arXiv:2306.01071. Bibcode:2023ApJ...949L..31Y. doi:10.3847/2041-8213/acd54b. ISSN 2041-8205.

Further reading

[edit]
Retrieved from "https://en.wikipedia.org/w/index.php?title=Galactic_Center_filament&oldid=1255825891"