G350.1-0.3

{{Infobox nebula

|name = G350.1-0.3

|image = G350.1-0.3 (NASA).jpg

|caption = Supernova remnant G350.1-0.3

|credit = NASA

|type = supernova remnant

|epoch = J2000

|class =

|ra = {{RA|17|21|01}}{{cite simbad|title=MSC 350.1-0.3|accessdate=26 November 2017}}

|dec = {{DEC|-37|26.0}}

|dist_ly = 15000

|dist_pc = 4600

|dist_z =

|appmag_v =

|appdia =

|size_v =

|constellation = Scorpius

|radius_ly = 8

|radius_pc = 2

|dimensions =

|absmag_v =

|names =

}}

G350.1-0.3 is a supernova remnant which is located in the constellation Scorpius. It is in the Milky Way, and possibly associated with a neutron star (XMMU J172054.5-372652) formed in the same supernova explosion. The object was formerly mistakenly classified as a distant galaxy.{{Cite web |last=O'Neill |first=Ian |date=2008-06-11 |title=XMM-Newton Discovers Strange-Shaped Supernova Remnant |url=https://www.universetoday.com/14975/xmm-newton-discovers-strange-shaped-supernova-remnant/ |access-date=2024-09-06 |website=Universe Today |language=en-US}}

G350.1-0.3, a bright radio source in the inner Milky Way, was initially identified by comparing observations from the Molonglo Observatory Synthesis Telescope and Parkes Observatory and classified as a supernova remnant in publications from 1973{{Cite journal |last1=Clark |first1=D. H. |last2=Caswell |first2=J. L. |last3=Green |first3=Anne J. |date=November 1973 |title=New Galactic Supernova Remnants |journal=Nature |language=en |volume=246 |issue=5427 |pages=28–30 |doi=10.1038/246028a0 |bibcode=1973Natur.246...28C |issn=0028-0836}} and 1975.{{Cite journal |last1=Gaensler |first1=B. M. |last2=Tanna |first2=A. |last3=Slane |first3=P. O. |last4=Brogan |first4=C. L. |last5=Gelfand |first5=J. D. |last6=McClure-Griffiths |first6=N. M. |last7=Camilo |first7=F. |last8=Ng |first8=C.-Y. |last9=Miller |first9=J. M. |date=2008-06-10 |title=The (Re-)Discovery of G350.1-0.3: A Young, Luminous Supernova Remnant and Its Neutron Star |journal=The Astrophysical Journal |language=en |volume=680 |issue=1 |pages=L37–L40 |arxiv=0804.0462 |bibcode=2008ApJ...680L..37G |doi=10.1086/589650 |issn=0004-637X |s2cid=15762045}} However, later higher-resolution images in the mid-80s revealed an unexpected irregular morphology that differed substantially from other supernova remnant sources.{{Cite web |title=Detective astronomers unearth hidden celestial gem |url=https://www.esa.int/Science_Exploration/Space_Science/Detective_astronomers_unearth_hidden_celestial_gem |access-date=2024-09-06 |website=European Space Agency |language=en}} It was then argued that G350.1-0.3 was a radio galaxy or a galaxy cluster, resulting in a reclassification in which supernova remnant catalogues downgraded the object to "supernova remnant candidate" or dropped it completely; G350.1-0.3 was subsequently "forgotten".

Research published in 2008 combined archival data and new images from XMM-Newton, the European Space Agency's orbiting x-ray telescope, to demonstrate that G350.1-0.3 is a supernova remnant. The researchers determined that the object's odd shape resulted from exploding next to a dense gas cloud, approximately 15,000 light years from Earth, that prevented even expansion and produced its elongated shape. The researchers also determined that the nearby thermal X-ray source, XMMU J172054.5-372652, is a central compact object of the supernova.

G350.1-0.3 is eight light years across and about 900–1000 years old, making one of the youngest and brightest supernova remnants in the Milky Way. It is unlikely that humans would have seen the supernova explosion because intervening interstellar dust would have likely prevented its viewing from Earth.