Barred spiral galaxy
A barred spiral galaxy is a spiral galaxy with a central bar-shaped structure composed of stars. Bars are found in approximately two-thirds of all spiral galaxies.1 Bars generally affect both the motions of stars and interstellar gas within spiral galaxies and can affect spiral arms as well.1
Edwin Hubble classified spiral galaxies of this type as "SB" (spiral, barred) in his Hubble sequence, and arranged them into three 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. A fourth type, SBm, was subsequently created to describe somewhat irregular barred spirals, such as the Magellanic Cloud galaxies, 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: spiral galaxy, elliptical galaxy and irregular galaxy.
In 2005, observations by the Spitzer Space Telescope backed up previously collected evidence that suggested the Milky Way as a barred spiral galaxy. Observations by radio telescopes had for years suggested the Milky Way is barred, but Spitzer's vision in the infrared region of the spectrum has provided a more definite calculation.
Barred spiral galaxies are apparently predominant, with surveys showing that up to two-thirds of all spiral galaxies contain a bar.3 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.4 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.5
Bars are thought to be a temporary phenomenon in the life of spiral galaxies, the bar structure decaying over time, transforming the galaxy from a barred spiral to a "regular" spiral pattern. 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.6 Since so many spiral galaxies have a bar structure, it is likely that it is a recurring phenomenon 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.7
Recent studies have confirmed the idea that bars are a sign of galaxies reaching full maturity as the "formative years" end. A team led by Kartik Sheth of the Spitzer Science Center at the California Institute of Technology in Pasadena discovered that only 20 percent of the spiral galaxies in the distant past possessed bars, compared with nearly 70 percent of their modern counterparts.8
|This section is empty. You can help by adding to it. (July 2011)|
|This section requires expansion. (April 2010)|
|SB0-||SB0- is a type of lenticular galaxy|
|SB0||SB0 is a type of lenticular galaxy|
|SB0+||SB0+ is a type of lenticular galaxy|
|SB0/a||SB0/a can also be considered a type of barred lenticular galaxy|
|NGC 4314||SBa||This is actually an "SB(rs)a"clarification needed|
|NGC 4921||SBab||This is actually an "SB(rs)ab"clarification needed|
|Messier 95||SBb||This is actually an "SB(r)b"clarification needed|
|NGC 3953||SBbc||This is actually an "SB(r)bc"clarification needed|
|NGC 1073||SBc||This is actually an "SB(rs)c"clarification needed|
|Messier 108||SBcd||This is actually an "SB(s)cd"clarification needed|
|NGC 2903||SBd||This is actually an "SB(s)d"clarification needed|
|NGC 5398||SBdm||SBdm can also be considered a type of barred Magellanic spiral||This is actually an "SB(rs)dm"clarification needed|
|NGC 55||SBm||SBm is a type of Magellanic spiral (Sm)||This is actually an "SB(s)m"clarification needed|
|NGC 2217||SBa||Canis Major|
|Magellanic Clouds||SBm||Dorado, Tucana|
- Galaxy morphological classification
- Galaxy formation and evolution
- Lenticular galaxy
- Spiral galaxy
- Firehose instability
|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.
- 04/03/07: Hubble: Barred Spiral Galaxy NGC 1672
- D. Mihalas (1968). Galactic Astronomy. W. H. Freeman. ISBN 978-0-7167-0326-6.
- "Blue bursts of hot young stars". ESA/Hubble. Retrieved 3 April 2013.
- 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 Notice 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, Scientific American, October 2005
- Barred Spiral Galaxies are Latecomers to the Universe Newswise, Retrieved on July 29, 2008.