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Polarimetric line profiles for scattering off rotating disks
Vink, J.S.; Harries, T.J.; Drew, J.E. (2005) -
Pre-eclipse dips in the ultraviolet light curves of two eclipsing nova-like cataclysmic variables
Mason, K.O.; Drew, J.E.; Knigge, C. (1997)Observations of the eclipsing nova-like variables UX UMa and RW Tri with the Hubble Space Telescope reveal substantial orbital modulations in their UV light. These modulations have a minimum about a quarter of an orbital ... -
The Principes de Asturias nebula: a new quadrupolar planetary nebula from the IPHAS survey
Mampaso, A.; Corradi, R.L.M.; Viironen, K.; Leisy, P.; Greimel, R.; Drew, J.E.; Barlow, M.J.; Frew, D.J.; Irwin, J.; Morris, R.A.H.; Parker, Q.A.; Phillipps, S.; Rodriguez-Flores, E.R.; Zijlstra, A.A. (2006) -
Probing the circumstellar structure of Herbig Ae/Be stars
Vink, J.S.; Drew, J.E.; Harries, T.J.; Oudmaijer, R.D. (2002) -
Probing the circumstellar structure of pre-main sequence stars
Vink, J.S.; Drew, J.E.; Harries, T.J.; Oudmaijer, R.D. (2003) -
Probing the circumstellar structures of T Tauri stars and their relationship to those of Herbig stars
Vink, J.S.; Drew, J.E.; Harries, T.J.; Oudmaijer, R.D.; Unruh, Y.C. (2005) -
The properties of cataclysmic variables in photometric Ha surveys
Witham, A.R.; Knigge, C.; Gansicke, B.T.; Aungwerojwit, A.; Corradi, R.M.; Drew, J.E.; Greimel, R.; Groot, P.; Morales-Rueda, L.; Rodriguez-Flores, E.R.; Rodriguez-Gil, P.; Steeghs, D. (2006) -
The protoplanetary disks in the nearby massive star forming region Cygnus OB2
G. Guarcello, M.; J. Drake, J.; J. Wright, N.; Drew, J.E.; A. Gutermuth, R.; L. Hora, J.; Naylor, T.; Aldcroft, T.; Fruscione, A.; Garcia-Alvarez, D.; L. Kashyap, V.; King, R. (2013-08)The formation of stars in massive clusters is one of the main modes of the star formation process. However, the study of massive star forming regions is hampered by their typically large distances to the Sun. One exception ... -
QU Car: a very high luminosity nova-like binary with a carbon-enriched companion
Drew, J.E.; Hartley, L.E.; Long, K.S.; van der Walt, J. (2003) -
A radial velocity study of the companion to the central star of Abell 35
Gatti, A.A.; Drew, J.E.; Lumsden, S.; Marsh, T.R.; Moran, C.; Stetson, P. (1997)We report the results of a radial velocity study of BD - 22.3467 deg (LW Hya), the cool companion to the subdwarf central star of the planetary nebula Abell 35. Estimates for its radial velocity have been obtained by cross ... -
Radiation-driven accretion disk winds
Drew, J.E.; Proga, D. (2000)The concept of an ‘effective' Eddington limit as a lower bound on the system luminosity required for mass loss to be radiation pressure driven is discussed and shown to fall in the interesting regime for high-state ... -
A radiation-driven disc wind model for massive young stellar objects
Drew, J.E.; Proga, D.; Stone, J.M. (1998)A radiation-driven disk wind model is proposed that offers great promise of explaining the extreme mass loss signatures of massive young stellar objects (the BN-type objects and more luminous Herbig Be stars). It is argued ... -
Radiation-driven winds from luminous accretion discs
Proga, D.; Stone, J.M.; Drew, J.E. (1998)We study the two-dimensional, time-dependent hydrodynamics of radiation-driven winds from luminous accretion disks in which the radiation force is mediated primar- ily by spectral lines. We assume the disk is flat, Keplerian, ... -
Resolved polarization changes across H alpha in the classical T Tauri star RY Tauri
Vink, J.S.; Drew, J.E.; Harries, T.J.; Oudmaijer, R.D.; Unruh, Y.C. (2003) -
A Search for New Planetary Nebulae Located at Large Galactocentric Distances
Mampaso, A.; Viironen, K.; Corradi, R.L.M.; Drew, J.E.; Greimel, R.; Sabin, L. (Astronomical Society of the Pacific, 2007)We introduce the new Galactic Plane Hα survey IPHAS, present our PNe selection method, and discuss two examples of very distant new PNe. -
The second data release of the INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS DR2)
Barentsen, Geert; Farnhill, Hywel John; Drew, J.E.; Gonzalez-Solares, E.A.; Greimel, R.; Irwin, M.J.; Miszalski, Brent; Ruhland, Christine; Groot, P.; Mampaso, A.; Sale, S. E.; Henden, A.A.; Aungwerojwit, A.; Barlow, M.J.; Carter, P.R.; Corradi, R.L.M.; Drake, J. J.; Eisloffel, J.; Fabregat, J.; Gansicke, B.T.; Gentile Fusillo, N. P.; Greiss, S.; Hales, A.S.; Hodgkin, S.; Huckvale, L.; Irwin, J.; King, R.; Knigge, C.; Kupfer, T.; Lagadec, E.; Lennon, D.J.; Lewis, J.R.; Mohr-Smith, M.; Morris, R.A.H.; Naylor, T.; Parker, Q. A.; Phillipps, S.; Pyrzas, S.; Raddi, Roberto; Roelofs, G.; Rodriguez-Gil, P.; Sabin, L.; Scaringi, Simone; Steeghs, D.; Suso, J.; Tata, R.; Unruh, Y.C.; van Roestel, J.; Viironen, K.; Vink, J.S.; Walton, N.A.; Wright, Nick; Zijlstra, A.A. (2014-11-11)The INT/WFC Photometric Hα Survey of the Northern Galactic Plane (IPHAS) is a 1800 deg2 imaging survey covering Galactic latitudes |b| < 5° and longitudes ℓ = 30°–215° in the r, i, and Hα filters using the Wide Field Camera ... -
The separation of the stars in the binary nucleus of the planetary nebula Abell 35
Gatti, A.A.; Drew, J.E.; Oudmaijer, R.D.; Marsh, T.R.; Lynas-Gray, A.E. (1998)Using the Planetary Camera on board the Hubble Space Telescope we have measured the projected separation of the binary components in the nucleus of the planetary nebula Abell 35 to be larger than 0.08′′ but less than 0.14′′. ... -
The shaping of planetary nebula Sh 2-188 through interactionwith the interstellar medium
Wareing, C.J.; O'Brien, T.J.; Zijlstra, A.A.; Kwitter, K.B.; Irwin, J.; Wright, N.; Greimel, R.; Drew, J.E. (2006) -
The shock-excited P-Cygni nebula
Barlow, M.J.; Drew, J.E.; Meaburn, J.; Massey, R.M. (1994)We have obtained images in the [N II] λ6584 line of the nebula around the luminous blue variable star P Cygni, using a 4 arcsec wide occulting strip. A nearly circular inner nebula is found, containing many bright ... -
Soft x-ray observations of the early b-giants beta and epsilon CMA
Drew, J.E.; Denby, M.; Hoare, M.G. (1994)The study reports observations performed with the PSPC on board the Roentgensatellit (ROSAT) of the two nearby giant stars Beta CMa (B1 II-III) and Epsilon CMa (B2 II). Upper limits in the region of +/- 10 percent can be ...