{"title":"Y矮星发现太阳附近最寒冷亚恒星群的挑战","authors":"Sandy K. Leggett","doi":"arxiv-2409.06158","DOIUrl":null,"url":null,"abstract":"Stars form in the Galaxy with a wide range in mass. If the mass is below 7%\nof the Sun's, then the object does not become hot enough for stable hydrogen\nburning. These substellar objects are called brown dwarfs. Maps of the sky at\ninfrared wavelengths have found large numbers of brown dwarfs. However only 24\nobjects have been found (as of April 2017) that are cold enough to be\nclassified as \"Y dwarfs\": these have atmospheres that are cooler than 500 K (or\n200 C, 400 F) and have masses only 5 - 20 times that of Jupiter. The coolest Y\ndwarf currently known, discovered in 2014, has a temperature around freezing,\nhas a mass of about 5 Jupiter masses, and is only 2 pc away from the Sun. These\nsmall and cold objects are faint and difficult to find. This chapter describes\nthe discovery and characterization of the Y dwarfs. Finding more of these very\ncold planet-like brown dwarfs will require an as-yet unplanned space mission\nmapping large areas of sky at wavelengths around 5 microns.","PeriodicalId":501068,"journal":{"name":"arXiv - PHYS - Solar and Stellar Astrophysics","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Y Dwarfs: The Challenge of Discovering the Coldest Substellar Population in the Solar Neighborhood\",\"authors\":\"Sandy K. Leggett\",\"doi\":\"arxiv-2409.06158\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Stars form in the Galaxy with a wide range in mass. If the mass is below 7%\\nof the Sun's, then the object does not become hot enough for stable hydrogen\\nburning. These substellar objects are called brown dwarfs. Maps of the sky at\\ninfrared wavelengths have found large numbers of brown dwarfs. However only 24\\nobjects have been found (as of April 2017) that are cold enough to be\\nclassified as \\\"Y dwarfs\\\": these have atmospheres that are cooler than 500 K (or\\n200 C, 400 F) and have masses only 5 - 20 times that of Jupiter. The coolest Y\\ndwarf currently known, discovered in 2014, has a temperature around freezing,\\nhas a mass of about 5 Jupiter masses, and is only 2 pc away from the Sun. These\\nsmall and cold objects are faint and difficult to find. This chapter describes\\nthe discovery and characterization of the Y dwarfs. Finding more of these very\\ncold planet-like brown dwarfs will require an as-yet unplanned space mission\\nmapping large areas of sky at wavelengths around 5 microns.\",\"PeriodicalId\":501068,\"journal\":{\"name\":\"arXiv - PHYS - Solar and Stellar Astrophysics\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-10\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Solar and Stellar Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.06158\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Solar and Stellar Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.06158","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
摘要
银河系中形成的恒星质量范围很广。如果质量低于太阳质量的 7%,那么天体的温度就不足以稳定地燃烧氢气。这些亚恒星天体被称为褐矮星。红外线波长的天空地图已经发现了大量的褐矮星。然而,目前(截至2017年4月)只发现了24个冷到足以被归类为 "Y矮星 "的天体:这些天体的大气温度低于500开氏度(或200摄氏度,400华氏度),质量只有木星的5-20倍。目前已知最冷的Y矮星是在2014年发现的,其温度约为冰点,质量约为5个木星质量,距离太阳只有2 pc。这些又小又冷的天体很微弱,很难发现。本章介绍了 Y 矮星的发现和特征描述。要想找到更多这些类似于非常寒冷的行星的褐矮星,就需要执行一项尚未计划的太空任务,用 5 微米左右的波长绘制大面积的天空图。
Y Dwarfs: The Challenge of Discovering the Coldest Substellar Population in the Solar Neighborhood
Stars form in the Galaxy with a wide range in mass. If the mass is below 7%
of the Sun's, then the object does not become hot enough for stable hydrogen
burning. These substellar objects are called brown dwarfs. Maps of the sky at
infrared wavelengths have found large numbers of brown dwarfs. However only 24
objects have been found (as of April 2017) that are cold enough to be
classified as "Y dwarfs": these have atmospheres that are cooler than 500 K (or
200 C, 400 F) and have masses only 5 - 20 times that of Jupiter. The coolest Y
dwarf currently known, discovered in 2014, has a temperature around freezing,
has a mass of about 5 Jupiter masses, and is only 2 pc away from the Sun. These
small and cold objects are faint and difficult to find. This chapter describes
the discovery and characterization of the Y dwarfs. Finding more of these very
cold planet-like brown dwarfs will require an as-yet unplanned space mission
mapping large areas of sky at wavelengths around 5 microns.