Resolving the Optical Emission Lines of Ly$\alpha$ Blob ``B1'' at z = 2.38: Another Hidden Quasar
(2013)
Journal Article
Overzier, R., Nesvadba, N., Dijkstra, M., Hatch, N., Lehnert, M., Villar-Martín, M., …Zirm, A. (2013). Resolving the Optical Emission Lines of Ly$\alpha$ Blob ``B1'' at z = 2.38: Another Hidden Quasar. Astrophysical Journal, 771, Article 89. https://doi.org/10.1088/0004-637x/771/2/89
We have used the SINFONI near-infrared integral field unit on the Very Large Telescope to resolve the optical emission line structure of one of the brightest (L Lyα ≈ 1044 erg s–1) and nearest (z ≈ 2.38) of all Lyα blobs (LABs). The target, known in... Read More about Resolving the Optical Emission Lines of Ly$\alpha$ Blob ``B1'' at z = 2.38: Another Hidden Quasar.