Matches in SemOpenAlex for { <https://semopenalex.org/work/W3098367033> ?p ?o ?g. }
- W3098367033 endingPage "1448" @default.
- W3098367033 startingPage "1440" @default.
- W3098367033 abstract "Strong stellar magnetic fields are believed to truncate the inner accretion disks around young stars, redirecting the accreting material to the high latitude regions of the stellar surface. In the past few years, observations of strong stellar fields on T Tauri stars with field strengths in general agreement with the predictions of magnetospheric accretion theory have bolstered this picture. Currently, nothing is known about the magnetic field properties of younger, more embedded Class I young stellar objects. It is believed that protostars accrete much of their final mass during the Class I phase, but the physics governing this process remains poorly understood. Here, we use high-resolution near-infrared spectra obtained with NIRSPEC on Keck and with Phoenix on Gemini South to measure the magnetic field properties of the Class I protostar WL 17. We find clear signatures of a strong stellar magnetic field. Analysis of this data suggests a surface average field strength of 2.9 ± 0.43 kG on WL 17. We present our field measurements and discuss how they fit with the general model of magnetospheric accretion in young stars." @default.
- W3098367033 created "2020-11-23" @default.
- W3098367033 creator A5009359010 @default.
- W3098367033 creator A5047638862 @default.
- W3098367033 creator A5077870084 @default.
- W3098367033 creator A5090408772 @default.
- W3098367033 date "2009-07-14" @default.
- W3098367033 modified "2023-10-18" @default.
- W3098367033 title "FIRST MAGNETIC FIELD DETECTION ON A CLASS I PROTOSTAR" @default.
- W3098367033 cites W1589184716 @default.
- W3098367033 cites W1615130469 @default.
- W3098367033 cites W1642880642 @default.
- W3098367033 cites W1666704755 @default.
- W3098367033 cites W1857227750 @default.
- W3098367033 cites W1873283002 @default.
- W3098367033 cites W1964842941 @default.
- W3098367033 cites W1966244186 @default.
- W3098367033 cites W1967676215 @default.
- W3098367033 cites W1971840770 @default.
- W3098367033 cites W1973433671 @default.
- W3098367033 cites W1974689993 @default.
- W3098367033 cites W1978391636 @default.
- W3098367033 cites W1979218713 @default.
- W3098367033 cites W1980382910 @default.
- W3098367033 cites W1983993499 @default.
- W3098367033 cites W1984858292 @default.
- W3098367033 cites W1985646600 @default.
- W3098367033 cites W1989885283 @default.
- W3098367033 cites W1992296621 @default.
- W3098367033 cites W1993600492 @default.
- W3098367033 cites W1997757464 @default.
- W3098367033 cites W1998527497 @default.
- W3098367033 cites W2001892464 @default.
- W3098367033 cites W2002652997 @default.
- W3098367033 cites W2003639536 @default.
- W3098367033 cites W2004955121 @default.
- W3098367033 cites W2005302398 @default.
- W3098367033 cites W2007474830 @default.
- W3098367033 cites W2011924956 @default.
- W3098367033 cites W2012578543 @default.
- W3098367033 cites W2017234279 @default.
- W3098367033 cites W2023344645 @default.
- W3098367033 cites W2028004649 @default.
- W3098367033 cites W2032155631 @default.
- W3098367033 cites W2035864227 @default.
- W3098367033 cites W2038537998 @default.
- W3098367033 cites W2038684645 @default.
- W3098367033 cites W2040709382 @default.
- W3098367033 cites W2042336801 @default.
- W3098367033 cites W2044711498 @default.
- W3098367033 cites W2046793067 @default.
- W3098367033 cites W2049896064 @default.
- W3098367033 cites W2050340053 @default.
- W3098367033 cites W2053680061 @default.
- W3098367033 cites W2061195673 @default.
- W3098367033 cites W2071956358 @default.
- W3098367033 cites W2072468297 @default.
- W3098367033 cites W2074965692 @default.
- W3098367033 cites W2082546665 @default.
- W3098367033 cites W2085416326 @default.
- W3098367033 cites W2106141219 @default.
- W3098367033 cites W2114945401 @default.
- W3098367033 cites W2126700402 @default.
- W3098367033 cites W2130211162 @default.
- W3098367033 cites W2139669427 @default.
- W3098367033 cites W2142220522 @default.
- W3098367033 cites W2143232458 @default.
- W3098367033 cites W2144219585 @default.
- W3098367033 cites W2149808951 @default.
- W3098367033 cites W2152162454 @default.
- W3098367033 cites W2165489255 @default.
- W3098367033 cites W2169225437 @default.
- W3098367033 cites W2320120954 @default.
- W3098367033 cites W3023143186 @default.
- W3098367033 cites W3101059806 @default.
- W3098367033 cites W3101433878 @default.
- W3098367033 cites W3101911260 @default.
- W3098367033 cites W3103352958 @default.
- W3098367033 cites W3105270052 @default.
- W3098367033 cites W3106483981 @default.
- W3098367033 cites W3121947533 @default.
- W3098367033 cites W3151550628 @default.
- W3098367033 cites W4205574399 @default.
- W3098367033 doi "https://doi.org/10.1088/0004-637x/700/2/1440" @default.
- W3098367033 hasPublicationYear "2009" @default.
- W3098367033 type Work @default.
- W3098367033 sameAs 3098367033 @default.
- W3098367033 citedByCount "30" @default.
- W3098367033 countsByYear W30983670332012 @default.
- W3098367033 countsByYear W30983670332014 @default.
- W3098367033 countsByYear W30983670332015 @default.
- W3098367033 countsByYear W30983670332016 @default.
- W3098367033 countsByYear W30983670332017 @default.
- W3098367033 countsByYear W30983670332018 @default.
- W3098367033 countsByYear W30983670332019 @default.
- W3098367033 countsByYear W30983670332020 @default.
- W3098367033 countsByYear W30983670332021 @default.
- W3098367033 countsByYear W30983670332022 @default.