Binary planetary nebulae nuclei towards the Galactic bulge

The mixed chemistry phenomenon in Galactic Bulge PNe

(2009) J. V. Perea-Calderón et al.   ASTRONOMY & ASTROPHYSICS

Binary planetary nebulae nuclei towards the Galactic bulge

(2009) B. Miszalski et al.   ASTRONOMY & ASTROPHYSICS

THE OUTFLOWS AND THREE-DIMENSIONAL STRUCTURE OF NGC 6337: A PLANETARY NEBULA WITH A CLOSE BINARY NUCLEUS

(2009) Ma. T. García-Díaz et al.   ASTROPHYSICAL JOURNAL

A “FIREWORK” OF H2KNOTS IN THE PLANETARY NEBULA NGC 7293 (THE HELIX NEBULA)

(2009) M. Matsuura et al.   ASTROPHYSICAL JOURNAL

A long trail behind the planetary nebula HFG1 (PK 136+05) and its pre-cataclysmic binary central star V664 Cas

(2009) P. Boumis et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

The Origin and Shaping of Planetary Nebulae: Putting the Binary Hypothesis to the Test

(2009) Orsola De Marco   PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC

TheSpitzer/GLIMPSE Surveys: A New View of the Milky Way

(2009) Ed Churchwell et al.   PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC

BINARY CENTRAL STARS OF PLANETARY NEBULAE DISCOVERED THROUGH PHOTOMETRIC VARIABILITY. I. WHAT WE KNOW AND WHAT WE WOULD LIKE TO FIND OUT

(2008) Orsola De Marco et al.   ASTRONOMICAL JOURNAL

Discovery of eclipsing binary central stars in the planetary nebulae M 3-16, H 2-29, and M 2-19

(2008) B. Miszalski et al.   ASTRONOMY & ASTROPHYSICS

Line ratios from shocked cloudlets in planetary nebulae

(2008) A. C. Raga et al.   ASTRONOMY & ASTROPHYSICS

Multiple and Precessing Collimated Outflows in the Planetary Nebula IC 4634

(2008) Martín A. Guerrero et al.   ASTROPHYSICAL JOURNAL

The Formation of Crystalline Dust in AGB Winds from Binary-induced Spiral Shocks

(2008) Richard G. Edgar et al.   ASTROPHYSICAL JOURNAL

The True Shapes of the Dumbbell and the Ring

(2008) Sun Kwok et al.   ASTROPHYSICAL JOURNAL

MASH-II: more planetary nebulae from the AAO/UKST Hα survey

(2008) Brent Miszalski et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY