Publicaciones

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  • Supernovae 1989A, 1989B, 1989D
    IAUC 4760 available at Central Bureau for Astronomical Telegrams. IAUC 4760 available at Central Bureau for Astronomical Telegrams.
    Ruiz-Lapuente, P. et al.

    Fecha de publicación:

    3
    1989
    Número de citas
    2
  • Probabilities of filaments in a Poissonian distribution of points. I - Straight filaments
    Statistical techniques are devised to assess the likelihood of a Poisson sample of points in two and three dimensions, containing specific filamentary structures. For that purpose, Otto et al.'s (1986) expression for the probability density of clumps in a Poissonian distribution of points is generalized for any value of the density contrast. A way
    Betancort-Rijo, J. E.

    Fecha de publicación:

    3
    1989
    Número de citas
    5
  • A stellar disk perpendicular to the radio jet in B2 0034+25
    CCD surface photometry of the radio galaxy B2 0034+25 is reported. Fourier analysis of the intensity variations along a set of closely spaced elliptical contours fitted to the intensity distribution reveals a high positive cos 4-theta component in the inner 10 arcsecs. Subtraction of elliptical models of the stellar light shows the presence of a
    Gonzalez-Serrano, J. I. et al.

    Fecha de publicación:

    3
    1989
    Número de citas
    9
  • Supernovae 1989A in NGC 3687 and 1989B in NGC 3627
    IAUC 4740 available at Central Bureau for Astronomical Telegrams. IAUC 4740 available at Central Bureau for Astronomical Telegrams.
    Kidger, M. et al.

    Fecha de publicación:

    2
    1989
    Número de citas
    2
  • Quiescent and outburst photometry of the dwarf nova SS Cygni
    Photometric observations of a wide and a narrow outburst of the dwarf nova SS Cygni are used to test the hypothesis that the same mechanism is responsible for the wide outbursts of U Gem stars and the wide outbursts of SU UMa stars. A search for modulations at or near the orbital period of the SS Cygni outbursts was conducted, showing no
    Honey, W. B. et al.

    Fecha de publicación:

    2
    1989
    Número de citas
    19