The ARP 105 features star and gas tide tails that exceed 362,000 light years.
The elliptical galaxy NGC 3561B (top left) and the Spiral Galaxy NGC 3561A (bottom right) form the ongoing merger-sparking guitar shapes known comprehensively as ARP.
ARP 105 It is located approximately 400 million light years from Earth, in the constellation of Ursa major.
Also known as NGC 3561, it was discovered by British astronomer John Herschel on March 30, 1827.
It consists of two huge galaxies, the elliptical galaxy NGC 3561B and the Spiral Galaxy NGC 3561A.
“The ARP 105 is one of the brightest objects in the busy Galaxy Cluster Abell 1185,” Hubble Astronomers said in a statement.
“Abell 1185 is a chaotic cluster of at least 82 galaxies, many of which are not only interacting, but many wandering spherical clusters that are not gravity attached to a particular galaxy.”
The gravity dance between the NGC 3561B and NGC 3561A creates the features of an attractive collision galaxy.
“The giant tail is drawn from two galaxies by gravity interaction, embedding a cluster of stars and a galaxy of d star,” the astronomer said.
“The uniquely shaped arrangement of the galaxy and tail gives the grouping the nickname: guitar.”
“The long lanes of dark dust emerging from the NGC 3561b oval galaxy may be ingesting the bright blue region of star-forming at the bottom of the guitar known as Ambartsumian's Knot.”
“Ambartsumian's Knot is a tidal star galaxy. It is a type of star-forming system that develops from fragments of the tidal arms of interacting galaxies.”
“The two bright blue regions of star formation are evident in Hubble images at the edge of a distorted helical galaxy.”
“The region on the left of the spiral galaxy may be very similar to the knot of Ambartumian, the knot of intense star-forming knot caused by the merger.”
“The area on the right is still under investigation. It may be part of the collision, but its velocity and spectral data are different from the rest of the system, so it could be a galaxy in the foreground.”
“The thin, faint gas tips are barely visible that stretch between two galaxies.”
“These tendrils are of particular interest to astronomers as they may help define the timescale of this collision evolution.”
Source: www.sci.news
