Astronomers Have Detected RRLs of Carbon/Oxygen Ions for the First Time

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Astronomers Have Detected RRLs of Carbon/Oxygen Ions for the First Time
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For the first time ever, a research team from the Shanghai Astronomical Observatory (SHAO) of the Chinese Academy of Sciences has successfully detected radio recombination lines (RRLs) of ions heavier than helium using the TianMa 65-m Radio Telescope (TMRT). These lines were identified as belonging

The white line shows the RRLs of ions of C and/or O detected by TMRT. The green areas are the modeled emission of ion RRLs. The green dotted lines are the modeled emission, taking into account all RLLs and molecular lines. The background is the image of the heart-shaped Orion nebula , with Orion KL located within the lower-left bright region of M42, credit to Shawn Nielsen.

The researchers made this new discovery while searching for interstellar emission lines as part of an ongoing TMRT spectral line survey toward Orion KL. While identifying the Ka-band spectral lines of Orion KL, they found several broad line features that could not be assigned to any molecular“These line features have weak intensities but are already significant enough to be distinguished due to the high sensitivity of the spectrum.

In addition, they found marginal signals of alpha lines in the Q band and beta lines in the Ka band. They compared the spectra obtained on different days and found that the frequencies of the line features remained unchanged when corrected for the motion of the Earth, confirming that the ion RRLs originated from space.

Previously, RRLs were commonly defined as radio spectral lines, caused by transitions of high-n levels of atoms, that appeared after the recombination of singly ionized ions and electrons. But now, the researchers have detected tens of unblended ion RRLs simultaneously.

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