Zooming in on a surprising ring

Eso_potw2429a_1024

eso_potw2429a July 15th, 2024

Credit: ALMA (ESO/NAOJ/NRAO)/ESO/D. Liu et al.

This Picture of the Week shows the distant galaxy PJ0116-24, a so-called Hyper Luminous Infrared Galaxy (HyLIRG). HyLIRGs are incredibly bright galaxies, lit up by the extremely rapid star formation within them. But what triggers this? Previous studies suggested that such extreme galaxies must result from galaxy mergers. These galaxy collisions are thought to create dense gas regions in which rapid star formation is triggered. But isolated galaxies could also become HyLIRGs via internal processes alone, if star-forming gas is rapidly funneled towards the galaxy’s centre. In a new paper led by Daizhong Liu (Max-Planck Institute for Extraterrestrial Physics), observations from ESO’s Very Large Telescope (VLT) and the Atacama Large Millimetre/submillimetre Array (ALMA) were combined to study the motion of gas within PJ0116-24. ALMA traces cold gas, seen here in blue, whereas the VLT, with its new Enhanced Resolution Imager and Spectrograph (ERIS), traces warm gas, shown in red. Thanks to these detailed observations, the team discovered that the gas in this extreme galaxy was rotating in an organised fashion, rather than in the chaotic way expected after a galactic collision –– a surprising result! This shows convincingly that mergers aren’t always needed for a galaxy to become a HyLIRG. PJ0116-24 is so far away that its light took about 10 billion years to reach us. Luckily, a foreground galaxy (not shown here) acted as a gravitational lens, bending and magnifying the light of PJ0116-24 behind it into the Einstein ring seen here. This precise cosmic alignment allows astronomers to zoom in on very distant objects and see them in a level of detail that would otherwise be very hard to achieve. Links Side-by-side comparison of the VLT and ALMA images Research paper led by the MPE infrared group, the PASSAGES collaboration and the ERIS consortium

Provider: European Southern Observatory

Image Source: https://www.eso.org/public/images/potw2429a/

Curator: European Southern Observatory, Garching bei München, None, Germany

Image Use Policy: Creative Commons Attribution 4.0 International License

Image Details Image Details

Image Type
Observation
Object Name
PJ0116-24
Subject - Distant Universe
Galaxy > Activity > Ultraluminous
Eso_potw2429a_128
 

Position Details Position Details

Position (ICRS)
RA = 1h 16m 46.8s
DEC = -24° 37’ 2.0”
Orientation
North is up
Field of View
0.2 x 0.2 arcminutes
Constellation
Cetus

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue ALMA (Band 3) Millimeter (CO(3-2)) 2.7 mm
Red VLT (ERIS) Infrared (H-alpha) 2.0 µm
Spectrum_ir1
Blue
Red
Eso_potw2429a_1280
×
ID
potw2429a
Subject Category
D.5.3.4  
Subject Name
PJ0116-24
Credits
ALMA (ESO/NAOJ/NRAO)/ESO/D. Liu et al.
Release Date
2024-07-15T11:00:00
Lightyears
Redshift
Reference Url
https://www.eso.org/public/images/potw2429a/
Type
Observation
Image Quality
Distance Notes
Facility
Atacama Large Millimeter/submillimeter Array, Very Large Telescope
Instrument
Band 3, ERIS
Color Assignment
Blue, Red
Band
Millimeter, Infrared
Bandpass
CO(3-2), H-alpha
Central Wavelength
2700000, 2000
Start Time
Integration Time
Dataset ID
None, None
Notes
Coordinate Frame
ICRS
Equinox
J2000
Reference Value
19.195, -24.6172222
Reference Dimension
1768.0, 1768.0
Reference Pixel
884.0, 884.0
Scale
-1.416667e-06, 1.416667e-06
Rotation
0
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
Creator (Curator)
European Southern Observatory
URL
https://www.eso.org
Name
Email
Telephone
Address
Karl-Schwarzschild-Strasse 2
City
Garching bei München
State/Province
None
Postal Code
D-85748
Country
Germany
Rights
Creative Commons Attribution 4.0 International License
Publisher
European Southern Observatory
Publisher ID
eso
Resource ID
potw2429a
Metadata Date
2024-07-01T14:08:23+02:00
Metadata Version
1.1
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Detailed color mapping information coming soon...

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There is no distance meta data in this image.

 

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