{"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}
引用次数: 0
Abstract
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.