The atomic gas structure was discovered using the Five-hundred-meter Aperture Spherical Telescope.
Atomic gas is the fundamental material from which all galaxies are formed. The evolution of galaxies is primarily a process of accreting atomic gas from the intergalactic medium and transforming it into stars.
As a result, the observation and research of atomic gas in and around galaxies are critical to the study of galaxy formation and evolution models. Observing the 21-cm fine structure line emission of atomic hydrogen in the radio waveband is the most direct way to explore atomic gas.
Recent deep mapping observations of 21-cm line emission in the vicinity of the well-known compact group of galaxies “Stephan’s Quintet,” using the Five-hundred-meter Aperture Spherical Telescope’s (19-beam receiver) led by Xu Cong, a researcher from the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC), revealed a very large atomic gas structure with a length of about 2 million light-years (about 20 times the size of the Milky Way).
The discovery was recently published in the journal Nature.
FAST is currently the largest and most sensitive single-dish radio telescope in the world, and its 19-beam receiver is the largest L-band multi-beam feed array for 21-cm line observations. The full commissioning of the FAST 19-beam receiver opened a new window on atomic gas in the Universe, particularly for low-density diffuse gas far away from galaxies.
“This is the largest atomic gas structure ever found around a galaxy group,” said XU. The observations reached a sensitivity of 1σ=4.2×1016 cm-2 per channel (Δv=20 km s-1; angular-resolution=4′), making them currently the most sensitive observations of atomic hydrogen 21-cm line emission at this angular resolution.
Ever since its discovery by the French astronomer Edouard Stephan in 1877, Stephan’s Quintet has continued revealing puzzles related to the complex web of galaxy-galaxy and galaxy-intragroup medium interactions in the group.
The new observations show that large-scale, diffuse, low-density gas (with a column identity less than 1018cm-2) exists far away from the center of the group, and it is likely that the gas has been there for ~1 giga years. The observations challenge the current theory of galaxy-group formation/evolution because it is not clear how the low-density atomic gas can survive ionization by the intergalactic UV background on such a long time scale.
Reference: “A 0.6 Mpc H i structure associated with Stephan’s Quintet” by C. K. Xu, C. Cheng, P. N. Appleton, P.-A. Duc, Y. Gao, N.-Y. Tang, M. Yun, Y. S. Dai, J.-S. Huang, U. Lisenfeld, and F. Renaud, 19 October 2022, Nature.