Alma’s close-up view of the centre of galaxy NGC 1377 (upper left) reveals a swirling jet. In this colour-coded image, reddish gas clouds are moving away from us, bluish clouds towards us, relative to the galaxy’s centre. The Alma image shows light with wavelength around one millimetre from molecules of carbon monoxide (CO). A cartoon view (lower right) shows how these clouds are moving, this time seen from the side.  
​CTIO/H. Roussel et al./ESO (left panel); Alma/ESO/NRAO/S. Aalto (top right panel); S. Aalto (lower right panel)

Alma finds a swirling, cool jet that reveals a growing, supermassive black hole

A Chalmers-led team of astronomers have used the Alma telescope to make the surprising discovery of a jet of cool, dense gas in the centre of a galaxy located 70 million light years from Earth. The jet, with its unusual, swirling structure, gives new clues to a long-standing astronomical mystery – how supermassive black holes grow.

A team of astronomers led by Susanne Aalto, professor of radio astronomy at Chalmers, has used the Alma telescope (Atacama Large Millimeter/submillimeter Array) to observe a remarkable structure in the centre of the galaxy NGC 1377, located 70 million light years from Earth in the constellation Eridanus (the River). The results are presented in a paper published in the June 2016 issue of the journal Astronomy and Astrophysics.

“We were curious about this galaxy because of its bright, dust-enshrouded centre. What we weren’t expecting was this: a long, narrow jet streaming out from the galaxy nucleus”, says Susanne Aalto.

The observations with Alma reveal a jet which is 500 light years long and less than 60 light years across, travelling at speeds of at least 800 000 kilometres per hour (500 000 miles per hour).

Most galaxies have a supermassive black hole in their centres; these black holes can have masses of between a few million to a billion solar masses. How they grew to be so massive is a long-standing mystery for scientists.

A black hole’s presence can be seen indirectly by telescopes when matter is falling into it – a process which astronomers call “accretion”. Jets of fast-moving material are typical signatures that a black hole is growing by accreting matter. The jet in NGC 1377 reveals the presence of a supermassive black hole. But it has even more to tell us, explains Francesco Costagliola (Chalmers and ORA-INAF, Italy), co-author on the paper.

“The jets we usually see emerging from galaxy nuclei are very narrow tubes of hot plasma. This jet is very different. Instead it’s extremely cool, and its light comes from dense gas composed of molecules”, he says.

The jet has ejected molecular gas equivalent to two million times the mass of the Sun over a period of only around half a million years - a very short time in the life of a galaxy. During this short and dramatic phase in the galaxy’s evolution, its central, supermassive black hole must have grown fast.

“Black holes that cause powerful narrow jets can grow slowly by accreting hot plasma. The black hole in NGC1377, on the other hand, is on a diet of cold gas and dust, and can therefore grow – at least for now – at a much faster rate”, explains team member Jay Gallagher (University of Wisconsin-Madison). 

The motion of the gas in the jet also surprised the astronomers. The measurements with Alma are consistent with a jet that is precessing – swirling outwards like water from a garden sprinkler. 

“The jet’s unusual swirling could be due to an uneven flow of gas towards the central black hole. Another possibility is that the galaxy’s centre contains two supermassive black holes in orbit around each other”, says Sebastien Muller, Chalmers, also a member of the team.

The discovery of the remarkable cool, swirling jet from the centre of this galaxy would have been impossible without Alma, concludes Susanne Aalto.

“Alma’s unique ability to detect and measure cold gas is revolutionising our understanding of galaxies and their central black holes. In NGC 1377 we’re witnessing a transient stage in a galaxy’s evolution which will help us understand the most rapid and important growth phases of supermassive black holes, and the life cycle of galaxies in the universe”, she says.

Images

Download full-resulotion images from Flickr: https://www.flickr.com/photos/onsala/albums/72157670466962966

1. (top) Alma’s close-up view of the centre of galaxy NGC 1377 (upper left) reveals a swirling jet. In this colour-coded image, reddish gas clouds are moving away from us, bluish clouds towards us, relative to the galaxy’s centre. The Alma image shows light with wavelength around one millimetre from molecules of carbon monoxide (CO). A cartoon view (lower right) shows how these clouds are moving, this time seen from the side. The background colour image of NGC 1377 and its surroundings is a composite made from a visible light images taken at the CTIO 1.5-metre telescope by H. Roussel et al. (2006) (V filter), and in filters r and i by ESO’s VLT Survey Telescope [VST] 
Image credit: CTIO/H. Roussel et al./ESO (left panel); Alma/ESO/NRAO/S. Aalto (top right panel); S. Aalto (lower right panel)

2. Alma’s close-up view of the centre of galaxy NGC 1377 reveals a swirling jet. In this colour-coded image, reddish gas clouds are moving away from us, bluish clouds towards us, relative to the galaxy’s centre. The image shows light with wavelength around one millimetre from molecules of carbon monoxide (CO). 
Image credit: ALMA/ESO/NRAO/S. Aalto & F. Costagliola

3. This cartoon view shows how the clouds of material that make up the jet are moving outward from the central black hole, this time seen from the side. Red colours show clouds that are moving away from us, and blue colours show clouds that are moving towards us, relative to the black hole in the galaxy’s centre. 
Image credit: S. Aalto

4. The galaxy NGC 1377 lies 70 million light years from Earth, seen here beyond stars in our own galaxy. This colour composite of NGC 1377 and its surroundings is made from visible light images taken at the CTIO 1.5-metre telescope by H. Roussel et al. (2006) (V filter), and in filters r and i by ESO’s VLT Survey Telescope [VST] 
Image credit: CTIO/H. Roussel et al./ESO
More about the research

This research is presented in the article A precessing molecular jet signaling an obscured, growing supermassive black hole in NGC 1377?, published in the June 2016 issue of Astronomy and Astrophysics (http://dx.doi.org/10.1051/0004-6361/201527664).

The team is composed of Susanne Aalto (Chalmers), Francesco Costagliola (Chalmers and ORA-INAF, Italy), Sebastien Muller (Chalmers), K, Sakamoto (Institute of Astronomy and Astrophysics, Academia Sinica, Taipei, Taiwan), Jay S. Gallagher (Department of Astronomy, University of Wisconsin-Madison), K. Dasyra (National and Kapodistrian​ University of Athens, Greece), K. Wada (Kagoshima University, Japan), F. Combes (Paris Observatory, France), S. Garcia-Burillo (Observatorio Astronomico Nacional (OAN)-Observatorio de Madrid, Spain), L. E. Kristensen (Harvard-Smithsonian Center for Astrophysics, USA), S. Martin (European Southern Observatory, Joint Alma Observatory and IRAM, France), P. van der Werf (Leiden Observatory, Netherlands), A. S. Evans (University of Virginia and Virginia and National Radio Astronomy Observatory, USA) and J. Kotilainen (Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Finland).

More about Alma

Alma (Atacama Large Millimeter/submillimeter Array) — with its 66 gigantic 12-metre and 7-metre antennas - is an international astronomy facility located at 5000 metres altitude at Chajnantor in northern Chile. 

The Atacama Large Millimeter/submillimeter Array (Alma), an international astronomy facility, is a partnership of 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 National Science Council of Taiwan (NSC) and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).

Chalmers and Onsala Space Observatory have been involved in Alma since its inception; receivers for the telescope are one of many contributions. Onsala Space Observatory is host to the Nordic Alma Regional Centre, which provides technical expertise to the Alma project and supports astronomers in the Nordic countries in using Alma.

More about Onsala Space Observatory

Onsala Space Observatory is Sweden's national facility for radio astronomy. The observatory provides researchers with equipment for the study of the earth and the rest of the universe. In Onsala, 45 km south of Gothenburg, it operates two radio telescopes and a station in the international telescope Lofar. It also participates in several international projects. The observatory is hosted by Department of Earth and Space Sciences at Chalmers University of Technology, and is operated on behalf of the Swedish Research Council.

Contacts

Robert Cumming, communications officer, Onsala Space Observatory, Chalmers, +46 31-772 5500, +46 70-493 31 14, robert.cumming@chalmers.se

Susanne Aalto, professor in radio astronomy, Chalmers, +46 31 772 5506, susanne.aalto@chalmers.se




Published: Mon 04 Jul 2016. Modified: Wed 06 Jul 2016