Search Results - "RIBEIRO, V. A. R. M"

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    OPTICAL MORPHOLOGY, INCLINATION, AND EXPANSION VELOCITY OF THE EJECTED SHELL OF NOVA MONOCEROTIS 2012 by RIBEIRO, V A R M, Munari, U, VALISA, P

    Published in The Astrophysical journal (01-05-2013)
    “…The morphology of the ejected shell of the He/N Nova Monocerotis 2012 outburst was studied in detail. Synthetic line profile spectra were compared to the…”
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    Multiwavelength observations of nova SMCN 2016-10a – one of the brightest novae ever observed by Aydi, E, Page, K L, Kuin, N P M, Darnley, M J, Walter, F M, Mróz, P, Buckley, D A H, Mohamed, S, Whitelock, P, Woudt, P, Williams, S C, Orio, M, Williams, R E, Beardmore, A P, Osborne, J P, Kniazev, A, Ribeiro, V A R M, Udalski, A, Strader, J, Chomiuk, L

    “…Abstract We report on multiwavelength observations of nova Small Magellanic Cloud Nova 2016-10a. The present observational set is one of the most comprehensive…”
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    ON THE PROGENITORS OF GALACTIC NOVAE by DARNLEY, M. J, RIBEIRO, V. A. R. M, BODE, M. F, HOUNSELL, R. A, WILLIAMS, R. P

    Published in The Astrophysical journal (10-02-2012)
    “…Of the approximately 400 known Galactic classical novae, only 10 of them, the recurrent novae, have been seen to erupt more than once. At least eight of these…”
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    The morphology of the expanding ejecta of V2491 Cygni (2008 N.2) by Ribeiro, V. A. R. M., Darnley, M. J., Bode, M. F., Munari, U., Harman, D. J., Steele, I. A., Meaburn, J.

    “…Determining the evolution of the ejecta morphology of novae provides valuable information on the shaping mechanisms in operation at early stages of the nova…”
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    Radio light curves and imaging of the helium nova V445 Puppis reveal seven years of synchrotron emission by Nyamai, M M, Chomiuk, L, Ribeiro, V A R M, Woudt, P A, Strader, J, Sokolovsky, K V

    “…ABSTRACT V445 Puppis is the only helium nova observed to date; its eruption in late 2000 showed high velocities up to 8500 km s−1, and a remarkable bipolar…”
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    A recurrent nova super-remnant in the Andromeda galaxy by Darnley, M. J., Hounsell, R., O’Brien, T. J., Henze, M., Rodríguez-Gil, P., Shafter, A. W., Shara, M. M., Vaytet, N. M. H., Bode, M. F., Ciardullo, R., Davis, B. D., Galera-Rosillo, R., Harman, D. J., Harvey, E. J., Healy, M. W., Ness, J.-U., Ribeiro, V. A. R. M., Williams, S. C.

    Published in Nature (London) (01-01-2019)
    “…The accretion of hydrogen onto a white dwarf star ignites a classical nova eruption 1 , 2 —a thermonuclear runaway in the accumulated envelope of gas, leading…”
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    Properties, evolution and morpho-kinematical modelling of the very fast nova V2672 Oph (Nova Oph 2009), a clone of U Sco by Munari, U., Ribeiro, V. A. R. M., Bode, M. F., Saguner, T.

    “…Nova Oph 2009 (V2672 Oph) reached maximum brightness V= 11.35 on 2009 August 16.5. With observed t 2(V) = 2.3 and t 3(V) = 4.2 d decline times, it is one of…”
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    Photometric evolution, orbital modulation and progenitor of Nova Mon 2012 by Munari, U., Dallaporta, S., Castellani, F., Valisa, P., Frigo, A., Chomiuk, L., Ribeiro, V. A. R. M.

    “…We present and discuss accurate and densely mapped BVR C I C light curves of the neon Nova Mon 2012, supplemented by the evolution in Stromgren b and y bands…”
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    RADIO FREQUENCY MODELS OF NOVAE IN ERUPTION. I. THE FREE-FREE PROCESS IN BIPOLAR MORPHOLOGIES by RIBEIRO, V A R M, CHOMIUK, L, Munari, U, Steffen, W, Koning, N, O'Brien, T J, Simon, T, Woudt, P A, Bode, M F

    Published in The Astrophysical journal (01-09-2014)
    “…Observations of novae at radio frequencies provide us with a measure of the total ejected mass, density profile, and kinetic energy of a nova eruption. The…”
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    THE DISTANCE TO NOVA V959 MON FROM VLA IMAGING by Linford, J. D., Ribeiro, V. A. R. M., Chomiuk, L., Nelson, T., Sokoloski, J. L., Rupen, M. P., Mukai, K., O'Brien, T. J., Mioduszewski, A. J., Weston, J.

    Published in The Astrophysical journal (01-06-2015)
    “…ABSTRACT Determining reliable distances to classical novae is a challenging but crucial step in deriving their ejected masses and explosion energetics. Here we…”
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