The term “cosmic unicorn” does not refer to a mythological creature lost in space. In astrophysics, it designates compact objects whose properties challenge known theoretical models. Two celestial bodies bear this nickname for very different reasons: a black hole candidate located in the constellation of the Unicorn and an atypical radio emitter spotted by the CHIME telescope.
Mass gap and compact objects: what the cosmic unicorn reveals about stellar physics
When a massive star dies, its core collapses. Depending on its residual mass, it forms either a neutron star or a stellar black hole. Between these two categories lies an intermediate zone called the mass gap, where theory predicts few objects.
It is precisely in this zone that The Unicorn is located, a black hole candidate discovered in the constellation of the Unicorn (Monoceros). Its estimated mass places it between the heaviest neutron stars and the lightest stellar black holes. This position makes it a testbed for models of compact object formation.
To find information about Cosmic Unicorn and keep up with the news of these discoveries, the distinction between mass gap and classic categories serves as a useful starting point.

CHIME J1634+44: the dead star emitting unexplained radio signals
The second object nicknamed cosmic unicorn is referred to as CHIME J1634+44, named after the Canadian radio telescope that detected it. It is a dead star, but its precise classification remains open.
Its radio behavior is atypical. Unlike classic pulsars, whose rotation slows predictably, CHIME J1634+44 exhibits characteristics that do not match either the standard profile of a neutron star or that of a highly magnetized white dwarf.
Why the nature of this object remains debated
Three hypotheses coexist within the scientific community:
- A neutron star with an unusual magnetic field, which would alter the expected radio emission pattern.
- A magnetized white dwarf, which would be rare and challenge the boundary between these two types of compact objects.
- An object of yet unclassified type, also located in the mass gap or exhibiting a novel internal configuration.
None of these avenues has been definitively confirmed. The difficulty lies in the fact that radio observations alone are insufficient to make a determination. X-ray or gravitational wave data would be necessary to refine the diagnosis.
Multi-messenger observation: the tools that allow for resolution
The study of cosmic unicorns illustrates a methodological turning point in astrophysics. For a long time, each type of radiation (radio, visible, X-rays, gravitational waves) was captured by dedicated instruments, without systematic cross-referencing. The so-called multi-messenger approach now combines these sources to create a more complete picture of the same object.
The XRISM mission, for example, has enabled the observation of X-ray pulsars with fine spectral resolution. This type of data helps distinguish a neutron star from a magnetized white dwarf, as their high-energy signatures differ.
Complementarity between radio telescopes and space observatories
CHIME captures radio signals from the Canadian ground. To complement its observations, astrophysicists rely on orbital instruments capable of detecting X-rays or gamma rays emitted by these compact objects. It is the intersection of these data that allows for narrowing down the hypotheses regarding the nature of a given celestial body.
An article published by CERN Courier in September 2026 highlights that this progress improves the comparison between black holes, neutron stars, and electromagnetic phenomena, although it does not alone confirm the identity of CHIME J1634+44.

Constellation of the Unicorn: why this corner of the sky concentrates discoveries
The constellation of the Unicorn (Monoceros) occupies a region of the sky crossed by the Milky Way. This position makes it rich in young stars, nebulae, and stellar remnants. The density of observable objects in this region partly explains why several notable discoveries are located there.
The Unicorn directly derives its nickname from this constellation. The choice of the word “unicorn” in contemporary astrophysical vocabulary is not fanciful: it refers to the celestial position of the object, not to any resemblance to the mythical animal.
From medieval symbol to scientific designation
The word unicorn carries a long symbolic history. In medieval bestiaries, the unicorn represented purity and rarity. Tapestries, such as The Lady and the Unicorn, have made it a major cultural symbol. Today, the term retains this connotation of rarity when applied to an astrophysical object: a celestial body so atypical that it escapes existing classifications.
This lineage between ancient symbolism and modern scientific nomenclature is not coincidental. Astronomers regularly choose evocative nicknames to designate objects whose nature remains to be elucidated, and “unicorn” precisely conveys the idea of a unique specimen in its kind.
Upcoming observation campaigns, particularly those combining radio and X-ray data, should help clarify the exact nature of CHIME J1634+44. In the meantime, the cosmic unicorn remains what it has always been in human imagination: a rare object whose reality eludes as one attempts to grasp it.



