Astronomers have completed the largest survey to date of the faint outskirts of nearby galaxies, successfully testing a low-cost system for exploring these local stellar systems. R. Michael Rich of the University of California, Los Angeles led an international team carrying out a survey for the Haloes and Environments of Nearby Galaxies (HERON) collaboration, published in a paper in Monthly Notices of the Royal Astronomical Society. The team find that the diameters of the galactic outskirts – the haloes - appear to correlate with the brightness and type of galaxy.
The outer regions of galaxies contain ancient stars ejected in collisions with other galaxies, as well as stars that were among the first to form in the galaxy’s history. Understanding these regions helps trace the invisible dark matter structures enmeshed with the visible stars and gas that make up the most obvious component of a galaxy.
For the survey the team used a dedicated relatively small 28-inch (0.7-m) telescope based near Frazier Park, California; 119 galaxies were observed in the study, a larger data set than any previous survey of this type. Images were acquired using a CCD chip (similar to that found in digital cameras), with each pixel on the chip covering a larger area of sky than a similar system in larger telescopes. The result was that in a 1-hour exposure, the telescope reveals the faint shells and plumes ejected in galaxy collisions as clearly as a comparable length exposure on the 3.6-m Canada France Hawaii Telescope, or a total exposure time of 21 hours using a conventional amateur telescope. The total cost of the telescope system is economical too: roughly US$150,000 (£121,000) or less than 10% of the cost of similar competing projects.
“We were surprised at how powerful a telescope of such modest size could be”, said Rich. “There will be many interesting fish to catch in this particular bay of the cosmic ocean, offering a potential lifetime of studies with very large telescopes”, he added.
Noah Brosch, an astronomer at Tel Aviv University and a member of the team, is leading two additional studies of galaxy discs and galaxy groups, using an identical 28-inch telescope that is part of the HERON collaboration, at the Wise Observatory of Tel Aviv University, near Mitzpe Ramon, Israel. Brosch says: “The low surface brightness Universe hides many surprises amongst galaxies, small groups of galaxies, and giant clusters; we expect our two telescopes to make many discoveries.”
Code developed by Aleksandr Mosenkov of the Russian Academy of Sciences allowed the team to precisely measure the extent of the galaxies. The team found that diameter of a galaxy's halo is correlated with a galaxy's brightness; those galaxies brighter than the Milky Way (the galaxy we live in) show the largest haloes, some exceeding 600,000 light-years across - significantly larger than the Milky Way and its satellites. The largest haloes are found in the round, red galaxies known as giant elliptical galaxies (a good example is Messier 87, located in the Virgo cluster) that weigh as much as 1 million million Suns, but giant haloes can also be found in galaxies like the Milky Way that have a disc.
These very faint, distant stars may trace the extent of dark matter associated with these galaxies, a possibility that the team plans to explore in the future. The team had sought a connection between evidence of a galaxy collision and the amount of star formation observed in a galaxy, but none is seen: old, red and dead galaxies are as likely to have visible collisions as a disc galaxy with a youthful burst of star formation; instead, collisions are mostly found to have occurred in any galaxy more luminous than the Milky Way. “Previously a study like this would examine a handful of galaxies; a sample of this size is unprecedented”, said Mosenkov.
The trove of images is published in the paper, and shows previously unknown faint extensions and faint companion galaxies. Among the surprises is a dwarf galaxy of diameter 50,000 light years, orbiting the spiral galaxy NGC 7331. NGC 4762, a red disc galaxy in the Virgo cluster of galaxies is viewed edge-on, and has faint projections that completely change at low surface brightness levels, appearing like a shoe. NGC 3628 appears at first to look like the Milky Way on edge, but the survey images show its flat disc to be a small part of a system looking like a dog bone connected to a long streamer. The observations suggest that collisions of galaxies are ubiquitous, and can eject stars hundreds of thousands of light years from their galaxy of origin.
The team will place all of its science images into the NASA/IPAC Infrared Science Community Archive, including new observations of additional galaxies not discussed in the paper. In total, it is expected that data for over 150 galaxies will become available to anyone in the world.
The 0.7m telescope used by Rich was designed by James Riffle of Aguila, Arizona for the Astro Works corporation, but it is no longer in production. The system is novel in that the camera is placed at the “prime” focus, in front of the primary mirror.
Dr Robert Massey
Royal Astronomical Society
Mob: +44 (0)7802 877699
Dr R. Michael Rich
Research Astronomer, Adjunct Professor
Division of Astronomy, Department of Physics and Astronomy
University of California at Los Angeles
Tel: +1 310-794-5337
Dr Noah Brosch
Dept. of Astronomy and Astrophysics, and the Wise Observatory
Tel Aviv University, Tel Aviv 69978, Israel
Dr Aleksandr Mosenkov
Senior Researcher of the Central Astronomical Observatory of the Russian Academy of Sciences
Tel: +7 961 8080513
In addition to Rich, Henry Lee-Saunders, David G. Milewski, and M.L. Saadie of UCLA, Aleksandr Mosenkov (Central Astronomical Observatory of the RAS), Andreas Koch (University of Heidelberg), John Kormendy (University of Texas), Julia Kennefick and Mike Fusco (University of Arkansas), Laura Sales and Lydia Elias (University of California, Riverside), Michael Cooper and James Bullock (University of California, Irvine), Andreas Burkert (University of Munich), Michelle Collins (University of Surrey), David Thilker (Johns Hopkins University), David Reitzel (Griffith Observatory), and Laura de Groot (College of Wooster) participated in the study.
The new work appears in: “The haloes and environments of nearby galaxies (HERON) – I. Imaging, sample characteristics, and envelope diameters”, R. Michael Rich, A. Mosenkov, et al., Monthly Notices of the Royal Astronomical Society 490 (2019) (DOI: 10.1093/mnras/stz2106).
A copy of the paper is available from: https://doi.org/10.1093/mnras/stz2106
Science images from the survey will be placed in the NASA/IPAC Infrared Science Community Archive, and will be live from 1 November 2019 at: https://irsa.ipac.caltech.edu/data/HERON/overview.html
Notes for editors
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