Astronomers reveal true colours of evolving galactic beasts

Astronomers have identified a rare moment in the life of some of the universe’s most energetic objects. Quasars were first observed 60 years ago, but their origins still remain a mystery. Now researchers at Durham University, UK, have spotted what they suggest is a “brief transition phase” in the development of these galactic giants that could shed light on how quasars and their host galaxies evolve. The new research is published in Monthly Notices of the Royal Astronomical Society.

 

Red and blue quasars
Artist’s impression of red and blue quasars. Red quasar (left): A brief transitional phase where the nascent quasar is enshrouded in gas and dust. This phase appears to be associated with young jets and strong winds, which ultimately drive away the obscuring gas and dust. Blue quasar (right): An unobscured quasar with signatures of evolved jets and less extreme winds.
Credit
S. Munro

Quasars are powered by the energy from supermassive black holes at their centres as they feed on surrounding gases. They are thousands of times brighter than galaxies like our Milky Way and the majority are blue in colour. However, a significant number are red as they are viewed through huge clouds of dust and gas that obscure them from view.

 

The conventional view of red quasars is that they are actually blue quasars that are angled away from our line-of-sight. Instead, the Durham team has ruled this model out and have shown that red quasars are likely to be the result of a brief, but violent, phase in the evolution of galaxies when the black hole ejects a large amount of energy into the surrounding clouds of dust and gas. This injection of energy blows away the dust and gas to reveal a blue quasar.

 

Observations using radio telescopes support this theory by showing that black holes at the centre of red quasars produce a greater amount of radio emission than those at the centre of blue quasars.

 

Lead author Lizelke Klindt, a PhD researcher in Durham University’s Centre for Extragalactic Astronomy, said: “How quasars develop has been the cause of significant uncertainty.

 

‘What our results suggest is that quasars undergo a brief transition phase, changing colour from red to blue, when they emerge from the deep shroud of dust and gas surrounding them.

 

‘What we believe we are seeing is a rare but important step in the life of these galactic beasts during galaxy evolution when their black holes are starting to shape their environments.”

 

The researchers studied 10,000 red and blue quasars as they would have been seen seven to 11 billion years ago when the universe was relatively young using archival data from the Sloan Digital Sky Survey and the Very Large Array radio astronomy observatory.

 

They say their research could also tell us more about galaxy evolution. Co-author Professor David Alexander, Head of Astronomy, at Durham University, said: “We expect that during this transition phase the energy from the supermassive black hole will burn off the gas needed to form stars.

 

‘Without the gas the galaxy cannot continue to grow, so what we are possibly seeing is the start of a quasar effectively ending the life of the galaxy by destroying the very thing it needs to survive.”

Transition from red to blue quasars
An artist’s impression of the transition from red to blue quasars. Red and blue quasars are related within an evolutionary sequence that connects dust-obscured star formation with quasar activity through gas inflow via merging galaxies and outflows from the quasar. With this model the rare red quasar population represents a brief transitional phase between the starburst and the blue quasar phase during which winds and/or jets drive away the obscuring dust, revealing an unobscured blue quasar, and ultimately shutting down the star formation to form a dormant early-type galaxy.
Credits: Gemini Observatory, GMOS-South, NSF; https://www.pxwall.com/4k-high-definition-galaxy-wallpaper/; Adapted by S. Munro.

The researchers say the next step in their research is to use more in-depth data to understand the finer details of this transition phase.

 

The research was funded by a Faculty of Science Durham Doctoral Scholarship, the Science and Technology Facilities Council, a European Union COFUND/Durham Junior Research Fellowship and the Swiss National Science Foundation.

 

Media contacts

 

Durham University Marketing and Communications Office

Tel: +44 (0)191 334 6075

communications.team@durham.ac.uk

 

Robert Massey

Royal Astronomical Society

Tel: +44 (0)20 7292 3979

Mob: +44 (0)7802 877699

press@ras.ac.uk

 

Morgan Hollis

Royal Astronomical Society

Mob: +44 (0)7802 877700

press@ras.ac.uk

 

Science contacts

 

Lizelke Klindt

PhD researcher, Durham University’s Centre for Extragalactic Astronomy

lizelke.klindt@durham.ac.uk

Available for interview from Monday 5 August to Wednesday 7 August, 0900 to 1900 BST

 

Please note that Lizelke will be at a conference in Edinburgh during this time and will be presenting her results there on Thursday 8 August.

 

Professor David Alexander

Head of Astronomy

Durham University

d.m.alexander@durham.ac.uk

Available for interview on Monday 5 August to Wednesday 7 August

 

Please note that David is away from Durham University at this time so his availability might be intermittent.

 

Images and captions

 

A selection of images is available including:

 

Figure 1 - Red quasar: A brief transitional phase where the young quasar is enshrouded in gas and dust. This phase is potentially associated with young jets and strong winds, which ultimately drive away the obscuring dust. Credit: S. Munro.

 

Figure 2 - Blue quasar: An unobscured quasar with signatures of evolved jets and less extreme winds that ultimately shut down star formation. Credit: S. Munro.

 

Figure 3 - red vs blue quasar (annotatednot annotated): Red quasar: A brief transitional phase where the nascent quasar is enshrouded in gas and dust. This phase appears to be associated with young jets and strong winds, which ultimately drive away the obscuring gas and dust. Blue quasar: An unobscured quasar with signatures of evolved jets and less extreme winds. Credit: S. Munro.

 

Sequence image (annotated / not annotated): Red and blue quasars are related within an evolutionary sequence that connects dust-obscured star formation with quasar activity through gas inflow via merging galaxies and outflows from the quasar. With this model the rare red quasar population represents a brief transitional phase between the starburst and the blue quasar phase during which winds and/or jets drive away the obscuring dust, revealing an unobscured blue quasar, and ultimately shutting down the star formation to form a dormant early-type galaxy. Credits: Gemini Observatory, GMOS-South, NSFhttps://www.pxwall.com/4k-high-definition-galaxy-wallpaper/; Adapted by S. Munro.

 

Images are also available on request from Durham University Marketing and Communications Office on +44 (0)191 334 6075; communications.team@durham.ac.uk

 

Further information

 

The new work appears in “Fundamental differences in the radio properties of red and blue quasars: evolution strongly favoured over orientation”, Klindt L, et al, Monthly Notices of the Royal Astronomical Society, published by Oxford University Press. DOI: 10.1093/mnras/stz1771

 

A copy of this paper is available on request from Durham University Marketing and Communications Office on +44 (0)191 334 6075; communications.team@durham.ac.uk

 

Notes for editors

 

About Durham University

 

Durham University is a globally outstanding centre of teaching and research based in historic Durham City.

 

We are a collegiate university committed to inspiring our people to do outstanding things at Durham and in the world.

 

We conduct boundary-breaking research that improves lives globally and we are ranked as a world top 100 university with an international reputation in research and education (QS World University Rankings 2020).

 

Our commitment to providing a wider student experience that fosters participation and leadership at Durham and beyond means our graduates are among some of the most sought after in the world and we are ranked in the top 50 globally for the employability of our students by major companies (QS 2020).

 

We are a member of the Russell Group of leading research-intensive UK universities and we are consistently ranked as a top 10 university in national league tables (Times and Sunday Times Good University Guide, Guardian University Guide and The Complete University Guide).

 

More information about Durham University.

 

 

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Submitted by Robert Massey on Mon, 05/08/2019 - 07:55