NGC 1512

{{Short description|Galaxy in the constellation Horologium}}

{{Infobox Galaxy

| name = NGC 1512

| image = NGC1510, NGC 1512 - Noirlab2210a.jpg

| caption = NGC 1512 and NGC 1510 imaged by the Cerro Tololo Inter-American Observatory

| epoch = J2000

| type = SB(r)ab{{cite web

| title=NASA/IPAC Extragalactic Database

| work=Results for NGC 1512

| url=http://nedwww.ipac.caltech.edu/

| access-date=2006-11-25 }}

| ra = {{RA|04|03|54.3}}

| dec = {{DEC|-43|20|56}}

| dist_ly = {{convert|11.6|Mpc|Mly|abbr=on|lk=on}} {{hub|0.73}}{{cite web

| title=NASA/IPAC Extragalactic Database

| work=Results for NGC 1512, Co-Moving Radial Distance

| url=http://nedwww.ipac.caltech.edu/

| access-date=2014-12-18 }}

| z = 898 ± 3 km/s

| appmag_v = 11.1

| size_v = 8.9{{prime}} × 5.6{{prime}}

| size = 213,140 ly (65.38 kpc) (estimated)

| constellation name = Horologium

| names = PGC 14391

}}

NGC 1512 is a barred spiral galaxy approximately 38 million light-years away from Earth in the constellation Horologium. The galaxy displays a double ring structure, with a (nuclear) ring around the galactic nucleus and an (inner) further out in the main disk. The galaxy hosts an extended UV disc with at least 200 clusters with recent star formation activity. NGC 1512 is a member of the Dorado Group.{{Cite journal

| bibcode = 1989ApJS...69..809M

| date = April 1989

| journal = Astrophysical Journal Supplement Series

| volume = 69

| pages = 809–829

| doi = 10.1086/191328

| title = A catalog of southern groups of galaxies

| author = Maia, M. A. G. | author2 =da Costa, L. N. | author3 =Latham, David W.

| doi-access = free

}}

Gravitational interaction with NGC 1510

Gravitational tidal forces of NGC 1512 are influencing nearby dwarf lenticular galaxy NGC 1510. The two galaxies are separated by only ~5 arcmin (13.8 kpc),{{cite journal

|last1=Koribalski |first1=Bärbel S.

|last2=López-Sánchez |first2= Ángel R.

|date=2009

|title=Gas dynamics and star formation in the galaxy pair NGC 1512/1510

|journal=Monthly Notices of the Royal Astronomical Society

|volume=400 |issue=4 |pages=21

|doi=10.1111/j.1365-2966.2009.15610.x

|doi-access=free

|arxiv=0908.4128|bibcode=2009MNRAS.400.1749K|s2cid=9329781

}} and are in the process of a lengthy merger which has been going on for 400 million years.{{cite web|title=Galactic David and Goliath|url=https://www.spacetelescope.org/news/heic1712/|website=www.spacetelescope.org|access-date=27 November 2017|archive-url=https://web.archive.org/web/20171201032836/https://www.spacetelescope.org/news/heic1712/|archive-date=1 December 2017|url-status=dead}} At the end of this process NGC 1512 will have cannibalised its smaller companion.{{cite web|title=NGC 1512 and NGC 1510|url=http://sci.esa.int/hubble/59356-ngc-1512-and-ngc-1510/|website=sci.esa.int|access-date=27 November 2017|archive-url=https://web.archive.org/web/20171201032832/http://sci.esa.int/hubble/59356-ngc-1512-and-ngc-1510/|archive-date=1 December 2017|url-status=dead}}

Interaction between these two galaxies has triggered star formation activity in the outskirts of the disc and enhanced the tidal distortion in the arms of the NGC 1512. The interaction seems to occur in the north-western areas of the system because of the broadening of the H i arm and the spread of the UV-rich star clusters in this region.

Gallery

NGC 1512 and NGC 1510.jpg|NGC 1512 and its companion the dwarf galaxy NGC 1510.

Ngc1512 nasajpl.jpg|An ultraviolet image of NGC 1510 and NGC 1512 taken with GALEX. The image shows that NGC 1512 has spiral arms that extend well beyond its optical disk. Credit:GALEX/NASA/JPL-Caltech.

NGC 1512 (2).jpg|The galaxy seen by the Hubble Space Telescope.

NGC 1512 (weic2403i).jpg|NGC 1512 seen by the James Webb Space Telescope.

NGC 1512.jpg|The nuclear ring of NGC 1512 as imaged by the Hubble Space Telescope (HST).
Credit: HST/NASA/ESA.

See also

References

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