| TON 618 | |
|---|---|
[[File:  |1089px|alt=]]TON 618, imaged by theSloan Digital Sky Survey Data Release 9 (DR9). The quasar appears as the bright, bluish-white dot at the center. | |
| Observation data(Epoch J2000.0) | |
| Constellation | Canes Venatici |
| Right ascension | 12h 28m 24.9s[1] |
| Declination | +31° 28′ 38″[1] |
| Redshift | 2.219[1] |
| Distance | |
| Type | Quasar[1] |
| Apparent magnitude (V) | 15.9[1] |
| Notable features | Hyperluminous quasar in aLyman-alpha blob |
| Other designations | |
| FBQS J122824.9+312837, B2 1225+31, QSO 1228+3128, 7C 1225+3145, CSO 140, 2E 2728, Gaia DR1 4015522739308729728[1] | |
| See also:Quasar,List of quasars | |
TON 618 (abbreviation ofTonantzintla 618) is a hyperluminous,broad-absorption-line, radio-loudquasar, andLyman-alpha blob[2] located near the border of theconstellationsCanes Venatici andComa Berenices, with the projectedcomoving distance of approximately 18.2 billionlight-years from Earth.[a] It possesses one of themost massive black holes ever found, at 40.7 billionM☉[3] orc. 40 billion.[4]
Asquasars were not recognized until 1963,[5] the nature of this object was unknown when it was first noted in a 1957 survey of faint blue stars (mainlywhite dwarfs) that lie away from theplane of theMilky Way. On photographic plates taken with the 0.7 m Schmidt telescope at theTonantzintla Observatory inMexico, it appeared "decidedly violet" and was listed by the Mexican astronomers Braulio Iriarte and Enrique Chavira as entry number 618 in theTonantzintla Catalogue.[6]
In 1970, a radio survey atBologna inItaly discovered radio emissions from TON 618, indicating that it was a quasar.[7] Marie-Helene Ulrich then obtained opticalspectra of TON 618 at theMcDonald Observatory which showedemission lines typical of a quasar. From the highredshift of the lines Ulrich deduced that TON 618 was very distant, and hence was one of the most luminous quasars known.[8]
As a quasar, TON 618 is believed to be theactive galactic nucleus at the center of a galaxy, the engine of which is asupermassive black hole feeding on intensely hot gas and matter in anaccretion disc. Given its observed redshift of 2.219, the light travel time of TON 618 is estimated to be approximately 10.8 billion years. Due to the brilliance of the central quasar, the surrounding galaxy is outshone by it and hence is not visible from Earth. With anabsolute magnitude of −30.7, it shines with a luminosity of4×1040watts, or as brilliantly as 140 trillion times that of the Sun, making it one of the brightest objects in the known Universe.[1]
Like other quasars, TON 618 has a spectrum containingemission lines from cooler gas much further out than the accretion disc, in thebroad-line region. The size of the broad-line region can be calculated from the brightness of the quasar radiation that is lighting it up.[9] Shemmer and coauthors used both NV and CIV emission lines in order to calculate the widths of theHβ spectral line of at least 29 quasars, including TON 618, as a direct measurement of their accretion rates and hence the mass of the central black hole.[10]
The emission lines in the spectrum of TON 618 have been found to be unusually wide,[8] indicating that the gas is travelling very fast; thefull width half maxima of TON 618 has been the largest of the 29 quasars, with hints of 10,500 km/s speeds of infalling material by a direct measure of the Hβ spectral line, indication of a very strong gravitational force.[10] From this, the mass of the central black hole of TON 618 has been estimated to be at 66 billion M☉.[10] This is considered one of the highest masses ever recorded for such an object; higher than the mass of all the stars in theMilky Way galaxy combined, which is 64 billion M☉,[11] and 15,300 times more massive thanSagittarius A*, the Milky Way's central black hole. With such high mass, TON 618 may fall into a proposed new classification ofultramassive black holes.[12][13] A black hole of this mass has aSchwarzschild radius of 1,300AU (about 195 billion km or 0.02ly) which is more than 40 times the distance fromNeptune to the Sun.
A more recent measurement in 2019 by Ge and colleagues which utilizes the C IV emission line, an alternative spectral line to Hβ, using the same data reproduced by the earlier paper by Shemmer found a lower relative velocity of the surrounding gas of2,761±423 km/s, which indicate a lower mass for the central black hole at 40.7 billion M☉, consequentially lower than the previous estimate.[3]
The nature of TON 618 as aLyman-alpha emitter has been well documented since at least the 1980s.[14] Lyman-alpha emitters are characterized by their significant emission of theLyman-alpha line, an ultraviolet wavelength emitted by neutral hydrogen. Such objects, however, have been very difficult to study due to the Lyman-alpha line being strongly absorbed by air in theEarth's atmosphere, limiting study of Lyman-alpha emitters to those objects with high redshifts. TON 618, with its luminous emission of Lyman-alpha radiation along with its high redshift, has made it one of the most important objects in the study of theLyman-alpha forest.[15]
Observations made by theAtacama Large Millimeter Array (ALMA) in 2021 revealed the apparent source of the Lyman-alpha radiation of TON 618: an enormous cloud of gas surrounding the quasar and its host galaxy.[2] This would make it aLyman-alpha blob (LAB), one of the largest such objects yet known.
LABs are huge collections of gases, or nebulae, that are also classified as Lyman-alpha emitters. These enormous, galaxy-sized clouds are some of thelargest nebulae known to exist, with some identified LABs in the 2000s reaching sizes of at least hundreds of thousands oflight-years across.[16]
In the case of TON 618, the enormous Lyman-alpha nebula surrounding it has the diameter of at least 100 kiloparsecs (330,000 light-years), twice the size of theMilky Way.[2] The nebula consists of two parts: an inner molecular outflow and an extensive cold molecular gas in its circumgalactic medium, each having the mass of 50 billionM☉,[2] with both of them being aligned to theradio jet produced by the central quasar. The extreme radiation from TON 618 excites the hydrogen in the nebula so much that it causes it to glow brightly in the Lyman-alpha line, consistent with the observations of other LABs driven by their inner galaxies.[17] Since both quasars and LABs are precursors of modern-day galaxies, the observation on TON 618 and its enormous LAB gave insight to the processes that drive the evolution of massive galaxies,[2] in particular probing their ionization and early development.
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