Fraser Cain on Nostr: Cepheids are variable stars that change brightness in a well-established relationship ...
Cepheids are variable stars that change brightness in a well-established relationship between luminosity and pulsation period. They have been used to measure the Universe's expansion rate with increasing accuracy. A few Cepheids are in binary pairs with a companion star, providing a way to measure their mass. Only one double-Cepheid has ever been found in the Large Magellanic Cloud. In a new study, astronomers report finding nine new binary Cepheids.
https://arxiv.org/abs/2403.12390 Published at
2024-03-20 18:26:03Event JSON
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"content": "Cepheids are variable stars that change brightness in a well-established relationship between luminosity and pulsation period. They have been used to measure the Universe's expansion rate with increasing accuracy. A few Cepheids are in binary pairs with a companion star, providing a way to measure their mass. Only one double-Cepheid has ever been found in the Large Magellanic Cloud. In a new study, astronomers report finding nine new binary Cepheids.\n\nhttps://arxiv.org/abs/2403.12390\n\nhttps://m.universetoday.com/system/media_attachments/files/112/129/419/711/466/390/original/f9f424221b5a2ce4.jpg",
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