NGC 1409

{{Short description|Lenticular galaxy in the constellation Taurus}}

{{Infobox Galaxy

| name = NGC 1409

| image = NGC 1409HSTFull.jpg

| image_size = 250px

| caption = Hubble Space Telescope image of NGC 1410 (left) and NGC 1409 (right)
Credit: HST/NASA/ESA

| constellation name = Taurus

| epoch = J2000

| type = SB0 or SAB pec

| ra = {{RA|03|41|10.546}}

| dec = {{DEC|−01|18|10.12}}

| dist_ly =

| h_radial_v = {{val|7750|40|u=km/s}}

| appmag_v = 15.4

| size_v = {{nowrap|1′.0 × 0′.8}}

| notes = Interacting with NGC 1410

| names = {{odlist | NGC=1409 | PGC=13553 | UGC=2821 }}

}}

NGC 1409 is a quiescent lenticular galaxy in the equatorial constellation of Taurus. It was discovered by the German-born astronomer William Herschel on January 6, 1785. NGC 1409 is located in close proximity to the smaller Seyfert galaxy NGC 1410, and the two are strongly interacting. Their respective nuclei have a separation of just {{convert|7|kpc|kly|disp=out|abbr=on|lk=on}}, and they share a diffuse stellar envelope with a radius extending out to {{convert|15|kpc|kly|disp=out|abbr=on|lk=off}}.

The morphological classification of this galaxy most closely matches type SB0, which indicates a barred lenticular galaxy. There is a conspicuous pipeline of dust and gas being funneled to NGC 1409 from NGC 1410. This lane has a typical width of {{convert|100|pc|ly|disp=out|abbr=on|lk=off}}, passing to the north in front of NGC 1409 and then behind, becoming denser toward the galactic core. It has an estimated mass of {{val|3|e=8|ul=solar mass}} and is transferring mass at the estimated rate of 1.1–1.4 {{solar mass}} yr–1. However, there is no indications of recent star formation in NGC 1409 from this incoming material.

References

{{reflist|refs=

{{cite simbad

| title=NGC 1409 | access-date=2020-10-10 }}

{{cite web

| first=Courtney | last=Seligman

| url=https://cseligman.com/text/atlas/ngc14.htm#1409

| title=NGC Objects: NGC 1400–1449

| access-date=2020-10-09 }}

{{cite web

| title=HubbleSite – NewsCenter – Intergalactic 'Pipeline' Funnels Matter Between Colliding Galaxies

| url=http://hubblesite.org/newscenter/archive/releases/2001/02/fastfacts/

| access-date=2007-04-05 }}

{{cite web

| title=NASA/IPAC Extragalactic Database

| work=Results for NGC 1409

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

| access-date=2007-04-05 }}

{{cite journal

| title=Ongoing Mass Transfer in the Interacting Galaxy Pair NGC 1409/1410

| last=Keel | first=William C.

| journal=The Astronomical Journal

| volume=127 | issue=3 | pages=1325–1335 | date=March 2004

| arxiv=astro-ph/0311633 | bibcode=2004AJ....127.1325K

| doi=10.1086/381927 | s2cid=16772319 }}

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}}