Antennae Galaxies: Difference between revisions

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Revision as of 00:25, 10 November 2018 edit146.198.193.18 (talk) →General information: 10 years ago is not recent, and the paper concerned is not widely cited← Previous edit		Revision as of 00:25, 10 November 2018 edit undo146.198.193.18 (talk) →General information: removed out of place paragraph, obviously chucked in by someone without heed to flow or organisationTag: references removedNext edit →
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	The Antennae Galaxies are undergoing a galactic collision. Located in the ] with five other galaxies, these two galaxies are known as the Antennae Galaxies because the two long tails of ]s, ] ejected from the galaxies as a result of the collision resemble an ] ]. The ] of the two galaxies are joining to become one giant ]. Most galaxies probably undergo at least one significant collision in their lifetimes. This is likely the future of our ] when it ] with the ].		The Antennae Galaxies are undergoing a galactic collision. Located in the ] with five other galaxies, these two galaxies are known as the Antennae Galaxies because the two long tails of ]s, ] ejected from the galaxies as a result of the collision resemble an ] ]. The ] of the two galaxies are joining to become one giant ]. Most galaxies probably undergo at least one significant collision in their lifetimes. This is likely the future of our ] when it ] with the ].

		⚫	The Antennae galaxies also contain a relatively young collection of massive globular clusters that were possibly formed as a result of the collision between the two galaxies.<ref>{{Cite journal\|title=van den Bergh, How Did Globular Clusters Form?\|journal=The Astrophysical Journal\|volume=559\|issue=2\|pages=L113\|url=http://iopscience.iop.org/article/10.1086/323754/fulltext/\|doi=10.1086/323754\|arxiv=astro-ph/0108298\|year=2001\|last1=Van Den Bergh\|first1=Sidney\|bibcode=2001ApJ...559L.113V}}</ref> The young age of these clusters is in contrast to the average age of most known globular clusters, around 12 billion years old, with the formation of the globulars likely originating from shockwaves, generated by the collision of the galaxies, compressing large, massive molecular clouds. The densest regions of the collapsing and compressing clouds are believed to be the birthplace of the clusters.

	Five supernovae have been discovered in NGC 4038: ], ], ], ] and ].<ref>{{cite web		Five supernovae have been discovered in NGC 4038: ], ], ], ] and ].<ref>{{cite web
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	\| url= http://www.cbat.eps.harvard.edu/lists/Supernovae.html		\| url= http://www.cbat.eps.harvard.edu/lists/Supernovae.html
	\| accessdate= 2015-08-22}}</ref>		\| accessdate= 2015-08-22}}</ref>

	They are located 0.25° north of ] and 3.25° southwest of ].<ref name="o'meara">{{cite book \|title=The Caldwell Objects \|first=Stephen James \|last=O'Meara \|publisher=Cambridge University Press \|year=2002 \|pages=240–43 \|isbn=978-0-521-82796-6 \| url=https://books.google.com.au/books?id=3Hg6YHgx9nAC&pg=PA242}}</ref>

⚫	The Antennae galaxies also contain a relatively young collection of massive globular clusters that were possibly formed as a result of the collision between the two galaxies.<ref>{{Cite journal\|title=van den Bergh, How Did Globular Clusters Form?\|journal=The Astrophysical Journal\|volume=559\|issue=2\|pages=L113\|url=http://iopscience.iop.org/article/10.1086/323754/fulltext/\|doi=10.1086/323754\|arxiv=astro-ph/0108298\|year=2001\|last1=Van Den Bergh\|first1=Sidney\|bibcode=2001ApJ...559L.113V}}</ref> The young age of these clusters is in contrast to the average age of most known globular clusters, around 12 billion years old, with the formation of the globulars likely originating from shockwaves, generated by the collision of the galaxies, compressing large, massive molecular clouds. The densest regions of the collapsing and compressing clouds are believed to be the birthplace of the clusters.

	==Timeline==		==Timeline==

Revision as of 00:25, 10 November 2018

Antennae Galaxies
NGC 4038 (left) and NGC 4039 (right)
Observation data (J2000 epoch)
Constellation	Corvus
Right ascension	12 01 53.0 / 12 01 53.6
Declination	−18° 52′ 10″ / −18° 53′ 11″
Redshift	1642 ± 12 / 1641 ± 9 km/s
Distance	45 Mly / 65 Mly
Apparent magnitude (V)	11.2 / 11.1
Characteristics
Type	SB(s)m pec / SA(s)m pec
Size	500,000 ly (150 kpc)
Apparent size (V)	5′.2 × 3′.1 / 3′.1 × 1′.6
Notable features	Interacting galaxies
Other designations
Ringtail Galaxy, NGC 4038 / 4039, PGC 37967 / 37969, Arp 244, Caldwell 60/61, UGCA 264/265

The Antennae Galaxies, also known as NGC 4038/NGC 4039, are a pair of interacting galaxies in the constellation Corvus. They are currently going through a starburst phase, in which the collision of clouds of gas and dust, with entangled magnetic fields, causes rapid star formation. They were discovered by William Herschel in 1785.

General information

The Antennae Galaxies are undergoing a galactic collision. Located in the NGC 4038 group with five other galaxies, these two galaxies are known as the Antennae Galaxies because the two long tails of stars, gas and dust ejected from the galaxies as a result of the collision resemble an insect's antennae. The nuclei of the two galaxies are joining to become one giant galaxy. Most galaxies probably undergo at least one significant collision in their lifetimes. This is likely the future of our Milky Way when it collides with the Andromeda Galaxy.

The Antennae galaxies also contain a relatively young collection of massive globular clusters that were possibly formed as a result of the collision between the two galaxies. The young age of these clusters is in contrast to the average age of most known globular clusters, around 12 billion years old, with the formation of the globulars likely originating from shockwaves, generated by the collision of the galaxies, compressing large, massive molecular clouds. The densest regions of the collapsing and compressing clouds are believed to be the birthplace of the clusters.

Five supernovae have been discovered in NGC 4038: SN 1921A, SN 1974E, SN 2004GT, SN 2007sr and SN 2013dk.

Timeline

About 1.2 billion years ago, the Antennae were two separate galaxies. NGC 4038 was a barred spiral galaxy and NGC 4039 was a spiral galaxy. Before the galaxies collided, NGC 4039 was larger than NGC 4038. 900 million years ago, the Antennae began to approach one another, looking similar to NGC 2207 and IC 2163. 600 million years ago, the Antennae passed through each other, looking like the Mice Galaxies. 300 million years ago, the Antennae's stars began to be released from both galaxies. Today the two streamers of ejected stars extend far beyond the original galaxies, resulting in the antennae shape.

Within 400 million years, the Antennae's nuclei will collide and become a single core with stars, gas, and dust around it. Observations and simulations of colliding galaxies suggest that the Antennae Galaxies will eventually form an elliptical galaxy.

X-ray source

Areas containing large amounts of neon, magnesium, and silicon were found when the Chandra X-ray Observatory analyzed the Antennae Galaxies. These elements are necessary in order for planets that may contain life to form. The clouds imaged contain 16 times as much magnesium and 24 times as much silicon as the Sun.

Image gallery

ESO's VLT observes the Antennae Galaxies.
Antennae Galaxies composite of ALMA and Hubble observations

References

R. W. Sinnott, ed. (1988). The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer. Sky Publishing Corporation and Cambridge University Press. ISBN 0-933346-51-4.
^ "NASA/IPAC Extragalactic Database". Results for NGC 4038 / 4039. Retrieved 2006-12-07.
Astronomy Picture of the Day Archive (28 April 2017). "Exploring the Antennae". Retrieved 2018-05-01.
"Corvus". Universe Today. Retrieved 2006-12-07.
Van Den Bergh, Sidney (2001). "van den Bergh, How Did Globular Clusters Form?". The Astrophysical Journal. 559 (2): L113. arXiv:astro-ph/0108298. Bibcode:2001ApJ...559L.113V. doi:10.1086/323754.
"List of Supernovae". IAU Central Bureau for Astronomical Telegrams. Retrieved 2015-08-22.
J. E. Barnes; L. Hernquist (1992). "Dynamics of interacting galaxies". Annual Review of Astronomy and Astrophysics. 30 (1): 705–742. Bibcode:1992ARA&A..30..705B. doi:10.1146/annurev.aa.30.090192.003421.

Notes

The quoted size was based on an assumed distance of 60 million ly although a more recent study gives a less remote distance of 45 million ly, giving consequently smaller values for the size.

External links

v t e Caldwell catalogue
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See also	Messier Catalogue Catalogue of Nebulae and Clusters of Stars New General Catalogue Index Catalogue Revised New General Catalogue Herschel 400 Catalogue
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