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Two sub-Neptune exoplanets detected by astronomersTOI-6054, or TIC 392681545, is an F-type subgiant star located some 259 light years away, about 66% larger but only slightly more massive than the sun. Two transit signals have been identified in ...
This nova has a recurrent timescale of about four years—the third-shortest of any nova—and consists of a white dwarf and a companion red subgiant (a star much larger than the sun). It was discovered ...
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