The famous young variable stellar object T Tauri, prototype to the class of pre-main-sequence objects which bears its name. T Tauri is actually a 0´´.6-separation binary star, unresolved in this image. (The objects very near the star just east of north and just west of south are filter glint artifacts, not infrared companions of T Tau.) The nebula to the west (NGC 1555) is reflected light from T Tauri.
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This work has been released into the public domain by its copyright holder, Two Micron All Sky Survey (2MASS). This applies worldwide. Joissain maissa laki ei mahdollista tätä. Mikäli näin on: Two Micron All Sky Survey (2MASS) myöntää kaikille oikeuden käyttää tätä teosta mihin tahansa tarkoitukseen ilman minkäänlaisia ehtoja, ellei laki vaadi ehtojen asettamista.
Atlas Image [or Atlas Image mosaic] obtained as part of the Two Micron All Sky Survey (2MASS), a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.
Atlas Image [or Atlas Image mosaic] courtesy of 2MASS/UMass/IPAC-Caltech/NASA/NSF.
Original caption: The famous young variable stellar object '''T Tauri''', prototype to the class of pre-main-sequence objects which bears its name. T Tauri is actually a 0´´.6-separation binary star, unresolved in this image. (The objects very near the
Tämä tiedosto sisältää esimerkiksi kuvanlukijan, digikameran tai kuvankäsittelyohjelman lisäämiä lisätietoja. Kaikki tiedot eivät enää välttämättä vastaa todellisuutta, jos kuvaa on muokattu sen alkuperäisen luonnin jälkeen.