Astronomers Study Mysterious New Type of Cosmic Blast
When astronomers discovered a cosmic explosion in a galaxy nearly 200 million light-years from Earth last June 16, they soon realized it was something different. While still debating the details, scientists now believe they may have gotten their first glimpse of the birth of a powerful phenomenon seen throughout the Universe.
The explosion was discovered by the ATLAS all-sky survey system in Hawaii, and immediately got the attention of astronomers. First, it was unusually bright for a supernova explosion — a common source of such outbursts. In addition, it brightened, then faded, much faster than expected.
Half a year later, “despite being one of the most intensely studied cosmic events in history, watched by astronomers all over the world, we still don’t know what it is,” said Anna Ho, of Caltech, who led a team using the Atacama Large Millimeter/submillimeter Array (ALMA), in Chile, among other telescopes. The object, dubbed AT2018cow, “heralds a new class” of energetic cosmic blasts, Ho added.
The explosion’s unusual characteristics “were enough to get everybody excited,” said Raffaella Margutti, of Northwestern University, who led a team that used telescopes ranging from gamma rays to radio waves, including the National Science Foundation’s Karl G. Jansky Very Large Array (VLA), to study the object. “In addition, AT2018cow’s distance of 200 million light-years, is nearby, by astronomical standards,” making it an excellent target for study, Margutti said.
Astronomers are presenting their findings about the object at the American Astronomical Society’s meeting in Seattle, Washington.
After watching the object and measuring its changing characteristics with a worldwide collection of ground-based and orbiting telescopes, scientists still are not sure exactly what it is, but they have two leading explanations. It may be, they suspect, either a very unusual supernova, or the shredding of a star that passed too close to a massive black hole, called a Tidal Disruption Event (TDE). Researchers are quick to point out, however, that the object’s characteristics don’t match previously-seen examples of either one.
“If it is a supernova, then it is unlike any supernova we have ever seen,” Ho said. The object’s range of colors, or spectrum, she said, “doesn’t look like a supernova at all.” In addition, it was brighter in millimeter waves — those seen by ALMA — than any other supernova.
It also differs from previously-seen Tidal Disruption Events.
“It’s off-center in its host galaxy,” Deanne Coppejans, of Northwestern University, said, meaning it can’t be a star shredded by the supermassive black hole at the galaxy’s center. “If it’s a TDE, then we need an intermediate mass black hole to do the shredding, and those are expected to form in stellar clusters,” Kate Alexander, an Einstein Fellow at Northwestern, added. The problem with that, she pointed out, is that AT2018cow appears to be inside a high-density interstellar medium, which “is difficult to reconcile with the density of gas in stellar clusters.”
Most of the researchers agree that AT2018cow’s behavior requires a central source of ongoing energy unlike those of other supernova explosions. The best candidate, they said, is a black hole that is drawing material from its surroundings. The inflowing material forms a rotating disk around the black hole and that disk radiates prolific amounts of energy. This is the type of “central engine” that powers quasars and radio galaxies throughout the Universe as well as smaller examples such as microquasars.
When a star much more massive than the Sun ceases thermonuclear fusion and collapses of its own gravity, producing a “normal” supernova explosion, no such central engine is produced. However, in the extreme cases called hypernovas, which produce gamma ray bursts, such a central engine produces the superfast jets of material that generate the gamma rays. That engine, however is very short-lived, lasting only a matter of seconds.
If such a central engine powered AT2018cow, it lasted for weeks, making this event distinct from the collapse-induced explosions of supernovas and the more-energetic such explosions that produce gamma ray bursts. In the case of a TDE, the “engine” would come to life as the black hole drew in material from the star shredded by its gravitational pull.
Alternatively, the “engine” resulting from a supernova explosion might be a rapidly-rotating neutron star with an extremely powerful magnetic field — a magnetar.
“We know from theory that black holes and neutron stars form when a star dies, but we’ve never seen them right after they are born. Never,” Margutti said.
“This is very exciting, since it would be the first time that astronomers have witnessed the birth of a central engine,” Ho said.
However, because of AT2018cow’s strange behavior, the verdict still is unclear, the scientists said. The central energy source could be a powerful shock wave hitting a dense shell of material at the object’s core. Either the strange supernova or the TDE explanation still is viable, Ho’s team said.
The astronomers look forward to more work on AT2018cow and to more objects like it.
“During the first few weeks, this object was very bright at millimeter wavelengths, so that means that, with ALMA now available, we may be able to find and study others,” Ho said. “The peak strength of the radio emission starts at ALMA wavelengths, and only moved to VLA wavelengths after a few weeks,” she added.
This news article was originally published by the U.S. National Radio Astronomy Observatory.
Paper and Research Team
These observation results were presented in the 233rd American Astronomical Society in January 2019. Also the results will be published as Ho et al. “AT2018COW: A LUMINOUS MILLIMETER TRANSIENT” in the Astrophysical Journal.
The research team members are:
Anna Y. Q. Ho (Caltech), E. Sterl Phinney (Caltech), Vikram Ravi (Caltech/Harvard-Smithsonian Center for Astrophysics), S. R. Kulkarni (Caltech), Glen Petitpas (Harvard-Smithsonian Center for Astrophysics), Bjorn Emonts (National Radio Astronomy Obsevatory), V. Bhalerao (Indian Institute of Technology Bombay), Ray Blundell (Harvard-Smithsonian Center for Astrophysics), S. Bradley Cenko (NASA Goddard Space Flight Center/University of Maryland), Dougal Dobie (University of Sydney/CSIRO Astronomy and Space Science), Ryan Howie (Harvard-Smithsonian Center for Astrophysics), Nikita Kamraj (Caltech), Mansi M. Kasliwal (Caltech), Tara Murphy (University of Sydney), Daniel A. Perley (Liverpool John Moores University), T. K. Sridharan (Harvard-Smithsonian Center for Astrophysics), and Ilsang Yoon (National Radio Astronomy Observatory)
The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of the European Southern Observatory (ESO), the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the Ministry of Science and Technology (MOST) in Taiwan and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).
ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA.