University of Hertfordshire Research Archive

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        Brinks, E. (47)
        Elmegreen, B. (8)Elmegreen, D.M. (8)Kaufman, M. (8)Skillman, E.D. (7)Walter, F. (6)Klaric, M. (5)Klein, U. (5)Taylor, C.L. (5)Thomasson, M. (5)... View MoreDate Issued1999 (12)1998 (4)1997 (9)1996 (4)1995 (4)1994 (6)1993 (3)1992 (2)1991 (2)1990 (1)

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        Now showing items 1-10 of 47

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        Massive stars shaping the ISM:Hi holes and shells in nearby galaxies 

        Brinks, E.; Walter, F. (1999)
        Neutral hydrogen (H I) is a magnificent tool when studying the structure of the interstellar medium (ISM) as it is relatively easily observable and can be mapped at good spatial and velocity resolution with modern instruments. ...

        Panel Discussion: Star Formation in Early-Type Galaxies 

        Knapp, G.R.; Binette, L.; Bower, R.; Brinks, E.; Goudfrooij, P.; Hau, G.; Pogge, R.; Young, L.M. (Astronomical Society of the Pacific, 1999)
        A panel discussion on past and current star formation in early-type galaxies was held on the second day of the conference. The panelists were Luc Binette, Elias Brinks, Paul Goudfrooij, Lisa Young, George Hau, Rick Pogge ...

        Ocular Galaxies: NGC 2535 and its Starburst Companion NGC 2536 

        Brinks, E.; Kaufman, M.; Elmegreen, D.M.; Thomasson, M.; Elmegreen, B.; Struck, C.; Klaric, M. (The International Astronomical Union, 1999)

        HI properties of Low Surface Brightness dwarf and blue compact dwarf galaxies 

        Taylor, C.L.; Brinks, E.; Skillman, E.D. (Astronomical Society of the Pacific, 1999)
        We present high resolution (~15") VLA HI observations of one LSB dwarf galaxy and 5 Blue Compact Dwarfs. Previous works have emphasized the difference in the peak column density of the HI between the two types of galaxy. ...

        Study of the interacting system NGC 6845 

        Rodrigues, I.; Dottori, H.; Brinks, E.; Mirabel, F. (1999)
        We present optical spectroscopy, B, V , R, and I CCD photometry, and VLA neutral hydrogen observations of the interacting quartet NGC 6845, also know as Klemola 30. NGC 6845 A, the dominant component, sports a broad and ...

        Massive stars shaping the ISM:Hi holes and shells in nearby galaxies 

        Brinks, E.; Walter, F. (The International Astronomical Union, 1999)
        Neutral hydrogen (H I) is a magnificent tool when studying the structure of the interstellar medium (ISM) as it is relatively easily observable and can be mapped at good spatial and velocity resolution with modern instruments. ...

        The interacting galaxies NGC 5394/5395: a post-ocular galaxy and its ring/spiral companion 

        Kaufman, M.; Brinks, E.; Elmegreen, B.; Elmegreen, D.M.; Klaric, M.; Struck, C.; Thomasson, M.; Vogel, S. (1999)

        HI Observations of Early-Type Galaxies 

        del Rio, M.S.; Brinks, E.; Carral, P.; Cepa, J. (Astronomical Society of the Pacific, 1999)
        We present high resolution (15") HI observations of the S0 galaxy NGC 404. We derive an HI mass of MHi = 6.7 x 10???, in good agreement with previous measurements. The HI is distributed in a broad annulus (a doughnut) and ...

        Interaction Between NGC 5394 and NGC 5395 

        Kaufman, M.; Brinks, E.; Elmegreen, B.; Elmegreen, D.M.; Klaric, M.; Struck, C.; Thomasson, M.; Vogel, S. (Astronomical Society of the Pacific, 1999)
        The spiral galaxies NGC 5394/95 (at a distance of 47 Mpc) are involved in a recent, close, nonmerging encounter. The smaller galaxy, NGC 5394, has two long, fairly symmetric, open tidal arms (see Figure 1); in numerical ...

        Neutral Hydrogen (21 Centimeter) Absorption in Seyfert Galaxies: Evidence for Free-Free Absorption and Subkiloparsec Gaseous Disks 

        Gallimore, J.F.; Baum, S.A.; O'Dea, C.P.; Pedlar, A.; Brinks, E. (1999)
        Active galaxies are thought to be both fueled and obscured by neutral gas removed from the host galaxy and funneled into a central accretion disk. We performed a VLA imaging survey of 21 cm absorption in Seyfert and starburst ...
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