NGC 986

{{Short description|Barred spiral galaxy in the constellation Fornax}}

{{Infobox galaxy

| name = NGC 986

| image = NGC 986 - ESOs Potw1605a.tif

| image_size =

| upright = 1.5

| caption = NGC 986 taken by the FORS instrument on ESO’s VLT.

| alt =

| epoch = J2000

| pronounce =

| constellation name = Fornax

| ra = {{RA|02|33|34.349}}

| dec = {{DEC|−39|02|42.21}}

| z = 0.006606

| h_radial_v = {{val|1942|10|u=km/s|fmt=commas}}

| gal_v =

| dist_pc =

| dist_ly = {{cvt|23.2|Mpc|Mly|order=flip|lk=on}}
56 million ly

| group_cluster = Fornax Cluster

| type = (R′1)SB(rs)b

| mass =

| mass_light_ratio =

| size =

| stars =

| appmag_v = 10.9

| appmag_b = 11.74

| absmag_v =

| size_v = {{nowrap|3′.8 × 1′.9}}

| half_light_radius_pc =

| half_light_radius_arcminsec =

| h1_scale_length_pc =

| h1_scale_length_arcminsec =

| xray_radius_pc =

| xray_radius_arcminsec =

| notes =

| names = {{odlist | NGC=986 | 2MASX=J02333434-3902422 | ESO=299-7 | HIPASS=J0233-39 | IRAS=02315-3915 | LEDA=9747 | MCG=-07-06-015 | NVSS=J023334-390237 }}

| references =

}}

NGC 986 is a barred spiral galaxy in the southern constellation of Fornax, located about 76 million light-years away. It was discovered on August 5, 1826, by the Scottish astronomer James Dunlop, who described it as a "faint nebula, of an irregular round figure". The galaxy has an angular size of {{nowrap|3′.8 × 1′.9}} with a visual magnitude of 10.9. It belongs to the Fornax Cluster of galaxies. This galaxy has a nearby companion, NGC 986A, at an angular separation of {{val|17|u=arcminute}}, corresponding to a projected separation of {{val|110|u=kpc}}. The two appear unconnected.

The morphological class of NGC 986 is (R′1)SB(rs)b, indicating this is a barred spiral (SB) with an outer pseudo-ring (R′1), an incomplete inner ring (rs), and moderately wound spiral arms (b). The galactic plane is inclined at an angle of 37° to the line of sight from the Earth. The resulting ellipsoidal profile has its major axis aligned along a position angle of 127°.

The nucleus of NGC 986 is undergoing intense star formation and there is an H II region at the core. The large central bar extends {{val|14|u=kpc|p=~}} and is rich in dense gas. The galaxy contains two large, extended and slightly warped arms that begin at each end of the central bar, forming an S-shape. There may be a tidally-disrupted dwarf galaxy at the end of its northern arm.

One supernova has been observed in NGC 986: SN 2018lei (type Ic, mag. 16.8).[https://www.wis-tns.org/object/2018lei Transient Name Server entry for SN 2018lei.] Retrieved 24 March 2023.

References

{{reflist|refs=

{{cite simbad

| title=NGC 986 | access-date=2022-01-11 }}

{{cite book

| title=Deep-Sky Companions: Southern Gems

| first=Stephen James | last=O'Meara

| date=2013 | page=44 | isbn=9781139851541

| publisher=Cambridge University Press

| url=https://books.google.com/books?id=BoIsCgAAQBAJ&pg=PA44 }}

{{cite journal

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| journal=The Astronomical Journal

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| doi=10.1086/375325 | bibcode=2003AJ....125.3005H | s2cid=122421859 | doi-access=free }}

{{cite journal

| title=The Two Micron All Sky Survey (2MASS)

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| last16=Seitzer | first16=Patrick | last17=Jarrett | first17=Thomas H.

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| journal=The Astronomical Journal

| date=1 February 2006 | volume=131 | issue=2 | pages=1163–1183

| bibcode=2006AJ....131.1163S | issn=0004-6256

| doi=10.1086/498708 | s2cid=18913331 | doi-access=free }}

{{cite journal

| title=ASTE CO(3-2) Observations of the Southern Barred Spiral Galaxy NGC 986: a Large Gaseous Bar Filled with a Dense Molecular Medium

| last1=Kohno | first1=Kotaro | last2=Tosaki | first2=Tomoka

| last3=Miura | first3=Rie | last4=Muraoka | first4=Kazuyuki

| last5=Sawada | first5=Tsuyoshi | last6=Nakanishi | first6=Kouichiro

| last7=Kuno | first7=Nario | last8=Sakai | first8=Takeshi

| last9=Sorai | first9=Kazuo | last10=Kamegai | first10=Kazuhisa

| last11=Tanaka | first11=Kunihiko | last12=Okuda | first12=Takeshi

| last13=Endo | first13=Akira | last14=Hatsukade | first14=Bunyo

| last15=Sameshima | first15=Masahiro | last16=Ezawa | first16=Hajime

| last17=Sakamoto | first17=Seiichi | last18=Kamazaki | first18=Takeshi

| last19=Yamaguchi | first19=Nobuyuki | last20=Cortés | first20=Juan

| last21=Tamura | first21=Yoichi | last22=Fukuhara | first22=Masayuki

| last23=Iono | first23=Daisuke | last24=Kawabe | first24=Ryohei

| journal=Publications of the Astronomical Society of Japan

| display-authors=1 | volume=60 | issue=3 | pages=457–464

| date=June 2008 | doi=10.1093/pasj/60.3.457

| arxiv=0805.1491 | bibcode=2008PASJ...60..457K }}

{{cite web

| title=An Often Ignored Beauty | date=1 February 2016

| url=http://www.eso.org/public/images/potw1605a/

| website=European Southern Observatory

| access-date=1 February 2016 }}

}}