A barred spiral galaxy is a spiral galaxy with a central bar-shaped structure composed of stars.[1] Bars are found in about half of all spiral galaxies.[2][3] Bars generally affect both the motions of stars and interstellar gas within spiral galaxies and can affect spiral arms as well.[2] The Milky Way Galaxy, where the Solar System is located, is classified as a barred spiral galaxy.[4]
Edwin Hubble classified spiral galaxies of this type as "SB" (spiral, barred) in his Hubble sequence and arranged them into sub-categories based on how open the arms of the spiral are. SBa types feature tightly bound arms, while SBc types are at the other extreme and have loosely bound arms. SBb-type galaxies lie in between the two. SB0 is a barred lenticular galaxy. A new type, SBm, was subsequently created to describe somewhat irregular barred spirals, such as the Magellanic Clouds, which were once classified as irregular galaxies, but have since been found to contain barred spiral structures. Among other types in Hubble's classifications for the galaxies are the spiral galaxy, elliptical galaxy and irregular galaxy.
Bars
Further information: Density wave theory § Galactic spiral arms
Barred spiral galaxy IC 5201, located more than 40 million light-years from Earth. It was discovered by Joseph Lunt.[5]
Barred galaxies are apparently predominant, with surveys showing that up to two-thirds of all spiral galaxies contain a bar.[6] The current hypothesis is that the bar structure acts as a type of stellar nursery, fueling star birth at their centers. The bar is thought to act as a mechanism that channels gas inwards from the spiral arms through orbital resonance, in effect funneling the flow to create new stars.[7] This process is also thought to explain why many barred spiral galaxies have active galactic nuclei, such as that seen in the Southern Pinwheel Galaxy.
The creation of the bar is generally thought to be the result of a density wave radiating from the center of the galaxy whose effects reshape the orbits of the inner stars. This effect builds over time to stars orbiting further out, which creates a self-perpetuating bar structure.[8]
Bars are thought to be temporary phenomena in the lives of spiral galaxies; the bar structures decay over time, transforming galaxies from barred spirals to more "regular" spiral patterns. Past a certain size the accumulated mass of the bar compromises the stability of the overall bar structure. Barred spiral galaxies with high mass accumulated in their center tend to have short, stubby bars.[9] Since so many spiral galaxies have bar structures, it is likely that they are recurring phenomena in spiral galaxy development. The oscillating evolutionary cycle from spiral galaxy to barred spiral galaxy is thought to take on the average about two billion years.[10]
Recent studies have confirmed the idea that bars are a sign of galaxies reaching full maturity as the "formative years" end. A 2008 investigation found that only 20 percent of the spiral galaxies in the distant past possessed bars, compared with about 65 percent of their local counterparts.[11]
Milky Way Galaxy spiral arms - based on WISE data.
Grades
NGC 7640 is a barred spiral galaxy in the Andromeda constellation.[12]
The general classification is "SB" (spiral barred). The sub-categories are based on how open or tight the arms of the spiral are. SBa types feature tightly bound arms. SBc types are at the other extreme and have loosely bound arms. SBb galaxies lie in between. SBm describes somewhat irregular barred spirals. SB0 is a barred lenticular galaxy.
Examples
Example | Type | Image | Information |
---|---|---|---|
NGC 2787 | SB0 | SB0 is a type of lenticular galaxy | |
NGC 4314 | SBa | ||
NGC 4921 | SBab | ||
Messier 95 | SBb | ||
NGC 3953 | SBbc | ||
NGC 1073 | SBc | ||
Messier 108 | SBcd | ||
NGC 2903 | SBd | ||
NGC 5398 | SBdm | SBdm can also be considered a type
of barred Magellanic spiral |
|
NGC 55 | SBm | SBm is a type of Magellanic spiral (Sm) |
Other examples
Name | Image | Type | Constellation |
---|---|---|---|
M58 | SBc | Virgo | |
M91 | SBb | Coma Berenices | |
M95 | SBb | Leo | |
M109 | SBb | Ursa Major | |
NGC 1300 | SBbc | Eridanus | |
NGC 7541 | SB(rs)bcpec | Pisces | |
NGC 1365 | SBc | Fornax | |
NGC 2217 | SBa | Canis Major | |
Magellanic Clouds | SBm | Dorado, Tucana | |
UGC 12158 | SB | Pegasus | |
NGC 1512[13] | SB(r)ab | Horologium |
See also
Astronomy portal
Galaxy morphological classification
Galaxy formation and evolution
Lenticular galaxy
Firehose instability
References
"Barred spiral galaxy". ScienceDaily. Retrieved 2018-09-17.
D. Mihalas (1968). Galactic Astronomy. W. H. Freeman. ISBN 978-0-7167-0326-6.
Timothy Ferris (1998). The Whole Shebang: A State-of-the-Universe(s) Report. Simon & Schuster. ISBN 978-0-6848-3861-8.
Gerhard, Ortwin (2002). "Mass distribution in our Galaxy". arXiv:astro-ph/0203110. (Sbc = spiral barred)
"A closer look at IC 5201". www.spacetelescope.org. Archived from the original on 15 December 2016. Retrieved 12 December 2016.
P. B. Eskridge; J. A. Frogel (1999). "What is the True Fraction of Barred Spiral Galaxies?". Astrophysics and Space Science. 269/270: 427–430. Bibcode:1999Ap&SS.269..427E. doi:10.1023/A:1017025820201.
J. H. Knapen; D. Pérez-Ramírez; S. Laine (2002). "Circumnuclear regions in barred spiral galaxies - II. Relations to host galaxies". Monthly Notices of the Royal Astronomical Society. 337 (3): 808–828. arXiv:astro-ph/0207258. Bibcode:2002MNRAS.337..808K. doi:10.1046/j.1365-8711.2002.05840.x.
F. Bournaud; F. Combes (2002). "Gas accretion on spiral galaxies: Bar formation and renewal". Astronomy and Astrophysics. 392 (1): 83–102. arXiv:astro-ph/0206273. Bibcode:2002A&A...392...83B. doi:10.1051/0004-6361:20020920.
Barred Spirals Come and Go, Sky and Telescope, April 2002
Ripples in a Galactic Pond Archived 2007-09-28 at the Wayback Machine, Scientific American, October 2005
Sheth, Kartik; Elmegreen, Debra Meloy; Elmegreen, Bruce G.; et al. (2008). "Evolution of the Bar Fraction in COSMOS: Quantifying the Assembly of the Hubble Sequence". The Astrophysical Journal. 675 (2): 1141–1155. arXiv:0710.4552. Bibcode:2008ApJ...675.1141S. doi:10.1086/524980. ISSN 0004-637X.
"A spiral in Andromeda". www.spacetelescope.org. Archived from the original on 7 February 2017. Retrieved 6 February 2017.
information@eso.org. "Galactic David and Goliath". www.spacetelescope.org. Archived from the original on 2017-09-22. Retrieved 2017-09-22.
External links
Wikimedia Commons has media related to Barred spiral galaxies.
Britt, Robert Roy. "Milky Way’s Central Structure Seen with Fresh Clarity." SPACE.com 16 August 2005.
An article about the Spitzer Space Telescope's Milky Way discovery
Devitt, Terry. "Galactic survey reveals a new look for the Milky Way." 16 August 2005.
The original press release regarding the article above, from the Univ. of Wisconsin
'Barred' Spiral Galaxy Pic Highlights Stellar Birth." SPACE.com 2 March 2001.
Hastings, George and Jane Hastings. Classifying Galaxies: Barred Spirals, 1995. "Astronomers Find Multiple Generations of Star Formation in Central Starburst Ring of a Barred Spiral Galaxy." January 15, 2000.
A press release concerning NGC 1326
Barred spirals come and go Sky & Telescope April 2002.
"ESO Provides An Infrared Portrait of the Barred Spiral Galaxy Messier 83." November 29, 2001.
A press release from the European Southern Observatory.
Horton, Adam. "Spitzer NGC 1291 barred spiral galaxy seen in infrared." 22 October 2014.
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Galaxies
Morphology
Disc Lenticular
barred unbarred Spiral
anemic barred flocculent grand design intermediate Magellanic unbarred Dwarf galaxy
elliptical irregular spheroidal spiral Elliptical galaxy
cD Irregular
barred Peculiar Ring
Polar
Structure
Active galactic nucleus Bar Bulge Dark matter halo Disc
Disc galaxy Halo
corona Galactic center Galactic plane Galactic ridge Interstellar medium Protogalaxy Spiral arm Supermassive black hole
Active nuclei
Blazar LINER Markarian Quasar Radio
X-shaped Relativistic jet Seyfert
Energetic galaxies
Lyman-alpha emitter Luminous infrared Starburst
blue compact dwarf pea faint blue Hot dust-obscured
Low activity
Low surface brightness Ultra diffuse Dark galaxy
Interaction
Field Galactic tide Cloud Groups and clusters
group cluster Brightest cluster galaxy fossil group Interacting
merger Jellyfish Satellite Stellar stream Superclusters Walls Voids and supervoids
void galaxy
Lists
Galaxies
Galaxies named after people Nearest Polar-ring Ring Spiral Groups and clusters Large quasar groups Quasars
Superclusters Voids
See also
Extragalactic astronomy Galactic astronomy Galactic coordinate system Galactic empire Galactic habitable zone Galactic magnetic fields Galactic orientation Galactic quadrant Galaxy color–magnitude diagram Galaxy formation and evolution Galaxy rotation curve Illustris project Intergalactic dust Intergalactic stars Intergalactic travel Population III stars
Hellenica World - Scientific Library
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