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  1. Home
  2. Browse by Author

Browsing by Author "Morelli, Lorenzo"

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    A colour-excess extinction map of the southern Galactic disc from the VVV and GLIMPSE surveys
    (2019) Soto, M.; Barba, R.; Minniti, D.; Kunder, A.; Majaess, D.; Nilo Castellon, J. L.; Alonso García, J.; Leone, G.; Contreras Ramos, Rodrigo Andrés; Hempel, Maren; Morelli, Lorenzo; Haikala, L.; Firpo, V.; Lucas, P.; Emerson, J. P.; Bidin, C. M.; Geisler, D.; Saito, R. K.; Gurovich, S.; Rejkuba, M.; Barbieri, M.; Román Lopes, A.; Alonso, M. V.; Baravalle, L. D.; Borissova, J.; Kurtev, R.; Milla, F
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    Light curves of type Ia supernovae from near the time of explosion
    (2007) Garg, Arti.; Morelli, Lorenzo; Clocchiatti, Alejandro; Minniti, D.
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    News from bulges hosted by low surface brightness galaxies
    (2006) Galaz, Gaspar; Lacerna Zambrano, Iván Andrés; Morelli, Lorenzo; Infante Lira, Leopoldo; Galaz, Gaspar; Lacerna Zambrano, Iván Andrés; Morelli, Lorenzo; Infante Lira, Leopoldo
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    Optical classification of 3 Swift southern hard X-ray sources
    (2006) Morelli, Lorenzo; Galaz, Gaspar; Morelli, Lorenzo; Galaz, Gaspar
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    Spectral identification of an ancient supernova using light echoes in the Large Magellanic Cloud
    (2008) Rest, A.; Morelli, Lorenzo; Pignata, Giuliano; Clocchiatti, Alejandro; Minniti, D.; Rest, A.; Morelli, Lorenzo; Pignata, Giuliano; Clocchiatti, Alejandro; Minniti, D.
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    The binary nucleus in VCC 128: A candidate supermassive black hole in a dwarf elliptical galaxy
    (2006) Debattista, Victor P.; Ferreras, Ignacio; Pasquali, Anna; Seth, Anil; De Rijcke, Sven; Morelli, Lorenzo
    Hubble Space Telescope (HST) Wide Field Planetary Camera 2 (WFPC2) images of the Virgo Cluster dwarf elliptical galaxy VCC 128 reveal an apparently double nucleus. The two components, which are separated by similar to 32 pc in projection, have the same magnitude and color. We present a spectrum of this double nucleus and show that it is inconsistent with one or both components being emission-line background objects or foreground stars. The most likely interpretation is that, as suggested by Lauer et al. for the double nucleus in NGC 4486B, we are seeing a nuclear disk surrounding a supermassive black hole. This is only the second time an early-type dwarf (dE/dSph) galaxy has been suggested to host a supermassive black hole.

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