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    Chapter and Conference Paper

    PRIME: A Deep Near-Infrared Survey Project

    PRIME is a proposed space mission for a deep survey of 25% to 100% of the sky in four near-IR bands (0.9-3.5 μm), to M AB ...

    A. Omont, W. Zheng, H. C. Ford, J. W. Kruk in Toward an International Virtual Observatory (2004)

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    Chapter and Conference Paper

    The nuclear spectrum of M 87

    The nuclear spectrum of M 87 covering the Lyα-Hα wavelength range was obtained with the HST Faint Object Spectrograph (FOS) trough a 0″.21 aperture. Contrary to some previous claims, a single power law (F ...

    Z. I. Tsvetanov, G. F. Hartig, H. C. Ford, G. A. Kriss in The Radio Galaxy Messier 87 (1999)

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    Chapter and Conference Paper

    Morphology of the nuclear disk in M 87

    A deep, fully sampled diffraction limited (FWHM ∼ 70 mas) narrowband image of the central region in M 87 was obtained with the Wide Filed and Planetary Camera 2 of the Hubble Space Telescope using the dithering t...

    Z. I. Tsvetanov, M. G. Allen, H. C. Ford, R. J. Harms in The Radio Galaxy Messier 87 (1999)

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    Article

    HST WFPC2 Line and Continuum Images of NGC 1068

    L.L. Dressel, Z.I. Tsvetanov, G.A. Kriss, H.C. Ford in Astrophysics and Space Science (1997)

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    Chapter and Conference Paper

    Imaging and Spectroscopy of Magellanic Cloud Planetary Nebulae obtained with the Hubble Space Telescope

    The majority of planetary nebulae (PNe) at the distance of the Magellanic Clouds typically subtend 1 arcsec or less on the sky. The Planetary Camera onboard the Hubble Space Telescope has a scale of 0.044 arcs...

    E. Vassiliadis, M. Dopita, R. C. Bohlin, J. P. Harrington in Planetary Nebulae (1997)

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    Chapter and Conference Paper

    Hubble Space Telescope Observations of Planetary Nebulae in the Magellanic Clouds

    We present the results of our major HST study of the evolution of PN in the Magellanic Clouds. This consists of imaging studies in [O III] and FOS UV spectroscopy. These data are then used in theoretical photo...

    M. A. Dopita, P. R. Wood, S. J. Meatheringham, E. Vassiliadis in Planetary Nebulae (1997)

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    Chapter and Conference Paper

    Planetary Nebulae and Halo Dynamics in Early Type Galaxies

    The study of extragalactic planetary nebulae has made rapid progress in recent years with the help of high quantum efficiency detectors. A brief but distinctive phase in the late stage of stellar evolution, pl...

    X. Hui, H. C. Ford in Planetary Nebulae (1993)

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    Chapter and Conference Paper

    Imaging of Magellanic Cloud Planetary Nebulae with the Hubble Space Telescope

    We have obtained Hubble Space Telescope (HST) Planetary Camera (PC) images of a number of Magellanic Cloud planetary nebulae. The objects, except for SMP 83 were observed as part of the Cycle I GO program. The...

    M. A. Dopita, S. J. Meatheringham, P. R. Wood, H. C. Ford in Planetary Nebulae (1993)

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    Article

    Human placental cytotrophoblast cells: identification and culture

    Methods of disaggregation of human placental tissue were assessed with the aim of maximising the yield of cytotrophoblast cells and minimising contamination with other cell types. Brief exposure to crude tryps...

    P. Truman, L. Pomare, H. C. Ford in Archives of Gynecology and Obstetrics (1989)

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    Chapter and Conference Paper

    Planetary Nebulae in Galaxies Beyond the Local Group

    Planetary nebulae can be used to estimate the distances to galaxies and to measure stellar dynamics in faint halos. We discuss surveys which have netted a total of 665 candidate planetary nebulae in NGC 5128 (...

    H. C. Ford, R. Ciardullo, G. H. Jacoby, X. Hui in Planetary Nebulae (1989)

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    Article

    The effect of substrate and epidermal growth factor on human placental trophoblast cells in culture

    Attempts were made to select for trophoblast cells in cultures of mixed cell populations derived from preterm (7 to 12 wk) or term human placentas. Epidermal growth factor added to cultures on solid or porous ...

    P. Truman, H. C. Ford in In Vitro Cellular & Developmental Biology (1986)

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    Chapter

    Dynamics of Some Remote Superclusters

    Redshifts of clusters of galaxies have been obtained in four regions of the sky selected as suspected rich superclusters at intermediate redshift (0.1 < z < 0.3). Measurements to date have detected the existen...

    R. J. Harms, H. C. Ford, R. Ciardullo in Early Evolution of the Universe and its Pr… (1983)

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    Article

    Thermal emission of Saturn's rings and disk at 34 µm

    OBSERVATIONS from aircraft of Saturn's thermal emission do not resolve the flux component of the rings from that of the planet1,2. Ground-based observations in the windows at 11 and 20 µm, which resolve the rings...

    I. G. NOLT, J. V. RADOSTITZ, R. J. DON NELLY, R. E. MURPHY, H. C. FORD in Nature (1974)