The very young star SU Aurigae has a protoplanetary disk with a tail
An article published in “The Astrophysical Journal Letters” reports a research on the very young star SU Aurigae, or simply SU Aur, and on the protoplanetary disk around it. A team of researchers used new observations conducted with the SPHERE instrument on the VLT, combining them with old observations conducted with the NaCo instrument, also on the VLT, with the Hubble Space Telescope, and with the ALMA radio telescope to study the disk. It has a sort of tail of dust that comes from a nebula that is probably the result of a collision between the star and a cloud of gas and dust.




