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  1. No Access

    Chapter

    ISO Observations of Symbiotic Stars

    A number of symbiotic stars have been observed with ISO. In addition to a number of emission lines, SWS observations of the symbiotic novae RR Tel and V1016 Cyg reveal prominent, broad 10 & 18 µm silicate dust fe...

    S. P. S. Eyres, A. Evans, A. Salama, P. Barr, J. Clavel in Astrophysics and Space Science (1998)

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    Chapter

    ISO Observations of Classical Novae

    We describe the ISO programme to observe classical novae. The programme includes observations of novae during and shortly after eruption, and old novae. ISO observations of far infrared fine structure lines ar...

    A. Salama, P. Barr, J. Clavel, R. N. Jenkins, K. Leech in Astrophysics and Space Science (1998)

  3. No Access

    Article

    ISO Observations of Symbiotic Stars

    A number of symbiotic stars have been observed with ISO. In addition to a number of emission lines, SWS observations of the symbiotic novae RR Tel and V1016 Cyg reveal prominent, broad 10 & 18 µm silicate dust...

    S.P.S. Eyres, A. Evans, A. Salama, P. Barr, J. Clavel in Astrophysics and Space Science (1997)

  4. No Access

    Article

    ISO Observations of Classical Novae

    We describe the ISO programme to observe classical novae. The programme includes observations of novae during and shortly after eruption, and old novae. ISO observations of far infrared fine structure lines ar...

    A. Salama, P. Barr, J. Clavel, R. N. Jenkins, K. Leech in Astrophysics and Space Science (1997)

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    Chapter and Conference Paper

    High-Resolution Spectroscopy of the Bright Quasar HS 1946+7658

    The optical spectrum of the QSO HS 1946+7658 (z em = 3.05) has been observed at high resolution (b ~ 15km/s) in the wavelength interval 4115 – 4970Å. Th...

    A. de la Fuente, Rodríguez-Pascual, J. L. Sanz, M. C. Recondo in QSO Absorption Lines (1995)

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    Chapter and Conference Paper

    The Lyα Forest towards HS1700+6416 at High Resolution

    We have analyzed high resolution (b ≈ 15 km/s) optical spectra of the QSO HS1700+6416 (z em = 2.72). The high S/N ratio in the Lyα forest allows a reasonable de...

    P. M. Rodríguez-Pascual, A. de la Fuente, J. L. Sanz, M. C. Recondo in QSO Absorption Lines (1995)

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    Chapter and Conference Paper

    Metal Line Absorptions Toward the QSO HS1700+6416

    We have analyzed high resolution (b ≈ 15 km/s) and low resolution (R ≈ 3Å) optical spectra of the QSO HS1700+6416 (z em = 2.72) taken with the ISIS spectrograph at the WHT. We are able to ...

    J. L. Sanz, P. M. Rodríguez-Pascual, A. de la Fuente, M. C. Recondo in QSO Absorption Lines (1995)

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    Chapter

    The International AGN Watch: A Multiwavelength Monitoring Consortium

    The International AGN Watch, an informal consortium of over 100 astronomers, was established to coordinate multiwavelength monitoring of a limited number of active galactic nuclei and thus obtain comprehensive...

    D. Alloin, J. Clavel, B. M. Peterson in Frontiers of Space And Ground-Based Astron… (1994)

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    Chapter

    The Infrared Space Observatory (ISO)

    The Infrared Space Observatory (ISO) is a three axis stabilized satellite designed to observe astronomical sources in the range 2.5–200 µm. It contains a cryogenically cooled telescope feeding four focal plane in...

    J. Clavel, M. F. Kessler in Frontiers of Space And Ground-Based Astronomy (1994)

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    Chapter and Conference Paper

    The Iue Ultraviolet Spectrum of PC 11

    PC 11 (HD 149427, PK 331–5 1) is classified as a young planetary nebula with strong OIII 4363Å and a Zanstra temperature of T Z = 27000K. It is also classified as (D’ - type) ye...

    M. Parthasarathy, S. R. Pottasch, J. Clavel in Planetary Nebulae (1993)

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    Chapter and Conference Paper

    FeII and Balmer continuum emission in AGNs

    We address in this short note a different aspect of the FeII problem in AGNs, one connected with treating the total FeII emission as a form of “continuum” rather than emission lines. The justification for this...

    R. Gilmozzi, W. Wamsteker, J. Clavel in Physics of Formation of FeII Lines Outside… (1988)

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    Chapter

    Discovery of Narrow and Variable Lines in the Ultraviolet Spectrum of the Seyfert Galaxy NGC 4151, and an Outline of Our Previous Results

    Extensive observations of NGC 4151 when the nucleus is at a minimum have led to the discovery of two emission lines which have a full width at half maximum of less than 7 and 16 Å respectively (after correctio...

    M. H. Ulrich, A. Altamore, A. Boksenberg in Structure and Evolution of Active Galactic… (1986)

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    Chapter

    T Cor B, a “Seyfert 1 Nucleus” at 1200±100 Parsecs?

    Several symbiotic stars are characterized by UV spectral signatures which are similar, in several aspects, to those observed in the broad-line region of Seyfert galaxies. We suggest to consider the symbiotic s...

    P. L. Selvelli, J. Clavel, A. Cassatella in Structure and Evolution of Active Galactic… (1986)

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    Chapter and Conference Paper

    Simultaneous Exosat-IUE Observations of NGC 4151

    NGC 4151 was observed four times in Nov. 83. The results indicate that: a) there exists a correlation between the X-ray and UV fluxes on the long term; b) the soft X-ray excess between 0.1 and 1 keV is probabl...

    G. C. Perola, A. Altamore, A. Boksenberg in X-Ray Astronomy in the Exosat Era (1985)

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    Chapter and Conference Paper

    Ultraviolet, Optical and X-Ray Monitoring of the Continuum of NGC 4151

    The nucleus of the Seyfert galaxy NGC 4151 has been extensively monitored with the International Ultraviolet Explorer (IUE) in the wave- length range 1200–3000 Å, a region of the spectrum where the contaminati...

    G. C. Perola, A. Boksenberg, G. E. Bromage, J. Clavel, M. Elvis in X-Ray Astronomy (1981)