Author´s Introduction

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In every ancient culture The Great Mother Goddess in Heaven was worshipped as showed here with the Egyptian picture 2 where you can see how life matter is formed and radiated out from her womb. The animated star atlas picture shows the centre in our Galaxy. 

The most common explanations of animal rock carvings having some drawings "inside" the body, are that the drawings are showing intestines which also can be the fact in some cases, but in many cases the interpreters are forgetting that there is mythological stories to tell when they are looking on the old rock carvings.

Picture 1 below with a crossed square on the back of the reindeer, marking the Galaxy centre, are from  Norway. Picture 2 are a star map marking the Galaxy centre with a red/blue swirl. Picture 3 are from Turkey showing the centre whit concentric rings and a dot.

Looking from our Sun system, the direction towards our Galaxy centre are placed in the star constellation of Sagittarius, here marked in the star map picture 2 with the red/blue swirl. Now if you think about the fact that the southern Milky Way contours was mythological interpreted both as a Woman and a Cow, you can se the resemblance between the pictures above and below.


Celtic art showing Universal creation patterns.

Bronze Age artefact from Finland illustrating the swirling force in Creation. Compare to my drawing to the right, the artefact are very likely to show the Solar System position in our Galaxy, The Milky Way.

Barred spiral galaxy


NGC 1300, viewed nearly face-on. Hubble Space Telescope image.

The Sculptor Galaxy, a barred spiral starburst galaxy, (2MASS).

A barred spiral galaxy is a spiral galaxy with a central bar-shaped structure composed of stars. Bars are found in approximately half 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 these types of spiral galaxies 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.

In 2005, observations by the Spitzer Space Telescope backed up previously collected evidence that suggested the Milky Way is a barred spiral galaxy. Observations by radio telescopes had for years suggested our galaxy to be barred, but Spitzer's vision in the infrared region of the spectrum has provided a more definite calculation.



The bars

Barred spiral galaxies are relatively common, with surveys showing that up to two-thirds of all spiral galaxies contain a bar.[2] 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.[3] 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.[4] Another possible cause of bar creation is gravitational disruptions between galaxies.[citation needed]

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. [5] 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.[6]

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.[7]

The bulges

Studying the core of the Milky Way, scientists found out that the Milky Way's bulge was peanut-shaped. This led to the conclusion that all barred spiral galaxies have a peanut shaped bulge. When observing a distant spiral galaxy with a rotational axis perpendicular to the line of sight, or one that appears "edge-on" to the observer, the shape of the bulge can be easily observed, and therefore quickly classified as either a barred spiral or a regular spiral. Galaxy NGC 4565 has been classified as an unbarred spiral galaxy using this method.[citation needed]










Coma Berenices






Ursa Major

NGC 1300



NGC 1365



Magellanic Clouds


Dorado, Tucana

See also


  1. ^ a b D. Mihalas (1968). Galactic Astronomy. W. H. Freeman. ISBN 9780716703266
  2. ^ P. B. Eskridge, J. A. Frogel (1999). "What is the True Fraction of Barred Spiral Galaxies?". Astrophysics and Space Science 269/270: 427–430. doi:10.1023/A:1017025820201. http://adsabs.harvard.edu/abs/1999Ap&SS.269..427E
  3. ^ 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. doi:10.1046/j.1365-8711.2002.05840.x. http://adsabs.harvard.edu/abs/2002MNRAS.337..808K
  4. ^ F. Bournaud, F. Combes (2002). "Gas accretion on spiral galaxies: Bar formation and renewal". Astronomy and Astrophysics 392: 83–102. doi:10.1051/0004-6361:20020920. http://adsabs.harvard.edu/abs/2002A&A...392...83B
  5. ^ Barred Spirals Come and Go, Sky and Telescope, April 2002
  6. ^ Ripples in a Galactic Pond, Scientific American, October 2005
  7. ^ Barred Spiral Galaxies are Latecomers to the Universe Newswise, Retrieved on July 29, 2008.

External links

Retrieved from "http://en.wikipedia.org/wiki/Barred_spiral_galaxy"

Categories: Barred spiral galaxies | Spiral galaxies | Barred galaxies | Galaxy morphological types