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| image = [[File:NGC 3114 Eguivar-crop.jpg|300 px]] | caption = Open cluster NGC 3114 in Carina ...

| name = [[New General Catalogue|NGC]] 4845 | caption = NGC 4845 as seen by [[Hubble Space Telescope|HST]] ...

| name = NGC 5679 | image = NGC 5679 Arp 274HST.jpg ...

| name=NGC 681 | image=File:NGC 681 legacy dr10.jpg ...

| name = NGC 596 | caption = [[Sloan Digital Sky Survey|SDSS]] image of NGC 596 ...

| title=Celestial Atlas: PCG Objects 24500–4999 ...p 9 ([[NGC 2523]]), Arp 10 ([[UGC 1775]]), Arp 11 (UGC 717), and Arp 12 ([[NGC 2608]]). ...

| name = [[New General Catalogue|NGC]] 6496 | image = [[File:NGC 6496.jpg|250px]] ...

| group_cluster = [[NGC 1407]]<ref name=paper/> ...-18|38|43}} ([[J2000]]). It is located within the [[Galactic corona]] of [[NGC 1407]], a massive [[spherical galaxy]] which is located approximately 163,0 ...

| name = [[New General Catalogue|NGC]] 1266 | image = File:NGC 1266 HST ACS.jpg ...

|image=[[File:NGC 1984 hst 08134 09 R814 G B555.png|280px]] |caption=The supergiant IRAS 05280–6910 in the open cluster [[NGC 1984]]. It is the bright reddened object near the centre ...

{{Short description|Disappearing red supergiant star in the galaxy NGC 6946 }} ...hreys|first=Roberta M.|date=2019-10-31|title=Comments on the Progenitor of NGC 6946-BH1|journal=Research Notes of the AAS|volume=3|issue=10|pages=164|doi= ...

...II. Are there really planets around IC 4651 No. 9122, NGC 2423 No. 3, and NGC 4349 No. 127? |journal=[[Astronomy & Astrophysics]] |volume=619 |issue= |pa [[Category:IC objects|4651]] ...

...the past this star has been considered a member of the [[open cluster]] [[NGC 1252]], but this now seems unlikely.<ref name=Marcos2013/> | title=NGC 1252: a high altitude, metal poor open cluster remnant ...

...e=variable/> It lies less than a degree from the small [[open cluster]] [[NGC 2645]], but is not a member.<ref name=aidelman/> ...l parameters of B stars in Collinder 223, Hogg 16, NGC 2645, NGC 3114, and NGC 6025|journal=Astronomy & Astrophysics|volume=577|pages=A45|last1=Aidelman|f ...

...2|M32]], [[Messier 81|M81]], [[Messier 82|M82]], [[Messier 87|M87]], and [[NGC 4151]].<ref>{{cite journal ...adsabs.harvard.edu/abs/1998AJ....115.2285M The Demography of Massive Dark Objects in Galaxy Centers], ''The Astronomical Journal'', '''115''', 2285-2305</ref ...

...htest star in this [[Sloan Digital Sky Survey]] image. The spiral galaxy [[NGC 47]] can be seen at upper left. ...{Cite simbad|title=BD-08 25|access-date=June 15, 2024}}</ref> The galaxy [[NGC 47]] lies just 320" from HD 984.<ref name=Coordinates/> ...

..., including [[globular clusters]] and [[planetary nebulae]]. Some of those objects were not visible at all on blue light (250–500&nbsp;nm) sensitive plates.<r ...iant Branch of the Elliptical Galaxy Maffei 1 and Comparisons with M32 and NGC 5128 | doi = 10.1086/342535 | journal = The Astronomical Journal | volume = ...

...ASS 08093547-4913033]], which is one of the M-dwarfs with a debris disk in NGC 2547 was observed with the [[Spitzer Space Telescope|Spitzer Infrared Spect ...ef name="Gaidos2022" /><ref name="Lee2020" /><ref name="Stahl2022" /> Some objects do not exactly fit the definition of Peter Pan disks, but are similar enoug ...

...s has been found in simulations with large number of gravitationally bound objects. ...t8=van de Ven |first8=Glenn |title=The Central Dark Matter Distribution of NGC 2976 |date=2012-01-03 |url=http://dx.doi.org/10.1088/0004-637x/745/1/92 |jo ...

...an SMC star, although the [[radial velocity]] is consistent with other SMC objects. The proper motion of around 10 mas/year would indicate a space velocity of ...e [[proper motion]]s and [[radial velocity]] are consistent with other SMC objects, while the parallax is negative but acceptably close to the expected value ...