Astronomers Discover Giant Relic of Disrupted "Tadpole" Galaxy

A team of astronomers from Israel, the U.S. and Russia have identified a disrupted galaxy resembling a giant tadpole, complete with an elliptical head and a long, straight tail, about 300 million light years away from Earth. The galaxy is one million light-years long from end to end, ten times larger than the Milky Way. The research is published today in the journal Monthly Notices of the Royal Astronomical Society.

 

The core of Hickson's Compact Group 98 consists of the two "smudges" at the centre of the image. Each is a galaxy much like our own Milky Way. The tadpole structure covers the central galaxy pair and was formed when the pair demolished a much smaller galaxy. The image was processed from the collection of the Stripe 82 project of the Instituto de Astrofisica de Canarias. Credit: N. Brosch / Tel Aviv University. Click for a larger image

“We have found a giant, exceptional relic of a disrupted galaxy,” says Dr Noah Brosch, of The Florence and George Wise Observatory at Tel Aviv University’s School of Physics and Astronomy, who led the research for the study.

 

When galaxies are disrupted and disappear, their stars are either incorporated into more massive galaxies or are ejected into intergalactic space. “What makes this object extraordinary is that the tail alone is almost 500,000 light-years long,” says Prof. R. Michael Rich of the University of California, Los Angeles. “If it were at the distance of the Andromeda galaxy, which is about 2.5 million light years from Earth, it would reach a fifth of the way to our own Milky Way.”

 

Drs Brosch and Rich collaborated on the study with Dr Alexandr Mosenkov of St. Petersburg University and Dr Shuki Koriski of TAU’s Florence and George Wise Observatory and School of Physics and Astronomy.

 

According to the study, the giant “tadpole” was produced by the disruption of a small, previously invisible dwarf galaxy containing mostly stars. When the gravitational force of two visible galaxies pulled on stars in this vulnerable galaxy, the stars closer to the pair formed the “head” of the tadpole. Stars lingering in the victim galaxy formed the “tail."

 

“The extragalactic tadpole contains a system of two very close ‘normal’ disc galaxies, each about 40,000 light-years across,” says Dr Brosch. “Together with other nearby galaxies, the galaxies form a compact group.” The galaxy is part of a small group of galaxies called HCG098 that will merge into a single galaxy in the next billion years.

 

Such compact galaxy groups were first identified in 1982 by astronomer Paul Hickson, who published a catalogue of 100 such groups. The Hickson Compact Groups examine environments with high galaxy densities that are not at the core of a “cluster” of galaxies (clusters contain thousands of galaxies themselves). The "tadpole galaxy" is listed as No. 98 in the Hickson Compact Group catalogue.

 

“In compact group environments, we believe we can study ‘clean’ examples of galaxy-galaxy interactions, learn how matter is transferred between the members, and how newly accreted matter can modify and influence galaxy growth and development,” says Dr Brosch.

 

For the research, the scientists collected dozens of images of the targets, each exposed through a wide filter that selects red light while virtually eliminating extraneous light pollution. “We used a relatively small, 70-cm telescope at the Wise Observatory and an identical telescope in California, both of which were equipped with state-of-the-art CCD cameras,” says Dr Brosch. The two telescopes are collaborating on a project called the Halos and Environments of Nearby Galaxies (HERON) Survey.

 

The new study is part of a long-term project at TAU’s Florence and George Wise Observatory, which explores the skies at low light levels to detect the faintest details of studied galaxies.

 

 

Media contacts

 

Ms Orna Cohen

Spokesperson’s Office

Tel Aviv University

ornac@tauex.tau.ac.il

 

Ms Daniella Alkobi

Account Director

Marino PR

Tel: +1 424 281 3789

dalkobi@marinopr.com

 

Dr Morgan Hollis

Royal Astronomical Society

Tel: +44 (0)20 7292 3977

Mob: +44 (0)7802 877 700

press@ras.ac.uk

 

 

Science contacts

 

Dr Noah Brosch

Tel Aviv University

Tel: +972 3 640 7413

Noah@wise.tau.ac.il

 

Prof. R. Michael Rich

University of California, Los Angeles

rmr@astro.ucla.edu

 

 

Images and captions

 

The core of Hickson's Compact Group 98 consists of the two "smudges" at the centre of the image. Each is a galaxy much like our own Milky Way. The point between them is a foreground star as are other circular features in the image. The tadpole structure covers the central galaxy pair and was formed when the pair demolished a much smaller galaxy. The image was processed from the collection of the Stripe 82 project of the Instituto de Astrofisica de Canarias. Credit: N. Brosch / Tel Aviv University

 

 

Further information

 

The new work appears in: “Hickson Compact Group 98: a Complex Merging Group with a Giant Tidal Tail and a Humongous Envelope”, N. Brosch, S. Koriski, R. Michael Rich, A.V. Mosenkov, Monthly Notices of the Royal Astronomical Society (2019), 482 (2) (DOI: 10.1093/mnras/sty2717).

 

A copy of the paper is available from: https://doi.org/10.1093/mnras/sty2717

 

 

Notes for editors

 

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Submitted by   on Fri, 26/10/2018 - 11:20