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Running out of gas: Gas loss puts breaks on stellar baby boom

Date:
August 2, 2017
Source:
National Astronomical Observatory of Japan
Summary:
Understanding the history of star formation in the Universe is a central theme in modern astronomy. Various observations have shown that the star formation activity has varied through the 13.8 billion-year history of the Universe. The stellar birthrate peaked around 10 billion years ago, and has declined steadily since then. However, the cause of the declining stellar birthrate is still not well understood.
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Understanding the history of star formation in the Universe is a central theme in modern astronomy. Various observations have shown that the star formation activity has varied through the 13.8 billion-year history of the Universe. The stellar birthrate peaked around 10 billion years ago, and has declined steadily since then. However, the cause of the declining stellar birthrate is still not well understood.

“Aiming to investigate what suppresses the star formation activity, we focused on the environment around the galaxies,” said Masao Hayashi at the National Astronomical Observatory of Japan (NAOJ).

Hayashi and his colleagues observed the galaxy cluster XMMXCS J2215.9–1738 located 9.4 billion light-years away [1] with the Atacama Large Millimeter/submillimeter Array (ALMA). Because it takes time for the light from distant objects to reach us, observing far-away galaxies shows us what the Universe looked like when the light was emitted. In this case, the light from XMMXCS J2215.9-1738 was emitted 9.4 billion years ago, which is around the time that the stellar birthrate peaked. In fact, previous observations with NAOJ’s Subaru Telescope revealed that many of the galaxies in the cluster are actively forming stars.

ALMA detected radio signals emitted from carbon monoxide gas in 17 of the galaxies in the cluster. This is a record-high number for the detection of gas-rich galaxies at such a distance. Interestingly, the gas-rich galaxies detected with ALMA are located towards the outer part of the galaxy cluster, not in the center. This is the first time ever that such a location differentiation has been found in a galaxy cluster 10 billion light-years away.

The team assumes that the gas-rich galaxies detected with ALMA are in an intermediate step in the process of becoming members of the cluster. As new member galaxies pass through the hot gas filling the cluster, cold gas in the galaxies is stripped away by the hot gas. Active star formation consumes what little gas survives in the galaxies. As the cold gas needed to make stars runs out, star formation stops.

Actually, there are some galaxies with active star formation at the central part of the cluster. The team suggests that they are rather evolved, old members of the cluster consuming the last of their gas to form stars.

“Recent observational and theoretical studies show that the distribution of gas is key to understanding the evolution of galaxies,” explains Hayashi. “Our observations provide robust statistics showing that a number of gas-rich galaxies are located in the outer part of a galaxy cluster. With this result we have opened a future path for revealing the evolutionary process of galaxies in galaxy clusters.”


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Materials provided by National Astronomical Observatory of Japan. Note: Content may be edited for style and length.


Journal Reference:

  1. Masao Hayashi, Tadayuki Kodama, Kotaro Kohno, Yuki Yamaguchi, Ken-ichi Tadaki, Bunyo Hatsukade, Yusei Koyama, Rhythm Shimakawa, Yoichi Tamura, Tomoko L. Suzuki. Evolutionary Phases of Gas-rich Galaxies in a Galaxy Cluster at z = 1.46. The Astrophysical Journal, 2017; 841 (2): L21 DOI: 10.3847/2041-8213/aa71ad

Cite This Page:

National Astronomical Observatory of Japan. "Running out of gas: Gas loss puts breaks on stellar baby boom." ScienceDaily. ScienceDaily, 2 August 2017. <www.sciencedaily.com/releases/2017/08/170802083312.htm>.
National Astronomical Observatory of Japan. (2017, August 2). Running out of gas: Gas loss puts breaks on stellar baby boom. ScienceDaily. Retrieved June 12, 2024 from www.sciencedaily.com/releases/2017/08/170802083312.htm
National Astronomical Observatory of Japan. "Running out of gas: Gas loss puts breaks on stellar baby boom." ScienceDaily. www.sciencedaily.com/releases/2017/08/170802083312.htm (accessed June 12, 2024).

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