Astronomers discover new brown dwarf with quasi-spherical mass loss

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Astronomers discover new brown dwarf with quasi-spherical mass loss
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Astronomers report the detection of a new brown dwarf as part of the Ophiuchus Disk Survey Employing ALMA (ODISEA) program. The newfound object, designated SSTc2d J163134.1-24006, appears to be experiencing a quasi-spherical mass loss. The discovery was detailed in a paper published September 2 on the arXiv pre-print repository.

Brown dwarfs are intermediate objects between planets and stars, occupying the mass range between 13 and 80 Jupiter masses . They can burn deuterium but are unable to burn regular hydrogen, which requires a minimum mass of at least 80 Jupiter masses and a core temperature of about 3 million K.led by Dary Ruiz-Rodriguez of the National Radio Astronomy Observatory in Charlottesville, Virginia, have investigated SSTc2d J163134.

"SSTc2d J163134.1 was observed as part of the 'Ophiuchus Disk Survey Employing ALMA' program . ALMA Band 6 observations were performed on April 27 and August 22, 2018, during Cycle 5 using the C43-3 configuration ," the researchers wrote in the paper. First of all, the team serendipitously discovered an expanding shell of carbon monoxide ejected from an object, with a temperature below 3,000 K, located in the direction of the Ophiuchus Molecular Cloud. Further observations revealed that this shell is associated with SSTc2d J163134.1.

In order to explain the nature of SSTc2d J163134.1 and its expanding shell, Ruiz-Rodriguez's team considered various scenarios, including the inside-out collapse of a dense molecular core in the Ophiuchus cloud, the mass loss of a giant star in the distant background, or a shell of gas expelled from a young brown dwarf. According to the researchers, the most plausible one is the brown dwarf hypothesis.

Given that emission of carbon monoxide from SSTc2d J163134.1 has an elliptical shape, it was noted that this makes it the first brown dwarf known to exhibit a quasi-spherical mass loss. The authors of the paper assume that a deuterium flash could be responsible for this phenomenon, but more detailed theoretical work is required in order to verify this explanation.

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