activity
20092012
most citedPrediction of close binarity based on planetary nebula morphology

7 citations · 9 across the 2 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2012

A study of the kinematics and binary-induced shaping of the planetary nebula HaTr 4

A. A. Tyndall, D. Jones, M. Lloyd +2

We present the first detailed spatio-kinematical analysis and modelling of the planetary nebula HaTr 4, one of few known to contain a post-common-envelope central star system. Comm…

astro-ph.SR2011

The morphology and kinematics of the Fine Ring Nebula, planetary nebula Sp 1, and the shaping influence of its binary central star

D. Jones, D. L. Mitchell, M. Lloyd +4

We present the first detailed spatio-kinematical analysis and modelling of the planetary nebula Shapley 1 (Sp 1), which is known to contain a close-binary central star system. Clos…

astro-ph.SR2010★ 2 cited

The binary central stars of PNe with the shortest orbital periods

M. Santander-Garcia, P. Rodriguez-Gil, D. Jones +4

Close binarity can play a significant role in the shaping of planetary nebulae (PNe) as the system evolves through the common-envelope phase. We present the detection of two of the…

astro-ph.SR2010★ 7 cited

Prediction of close binarity based on planetary nebula morphology

B. Miszalski, R. L. M. Corradi, D. Jones +3

A thorough search of the OGLE-III microlensing project has more than doubled the total sample of PNe known to have close binary central stars. These discoveries have enabled close…

astro-ph.SR2010

The Necklace: equatorial and polar outflows from the binary central star of the new planetary nebula IPHASXJ194359.5+170901

R. L. M. Corradi, L. Sabin, B. Miszalski +13

IPHASXJ194359.5+170901 is a new high-excitation planetary nebula with remarkable characteristics. It consists of a knotty ring expanding at a speed of 28 km/s, and a fast collimate…

astro-ph.SR2010

The kinematics of the quadrupolar nebula M1-75 and the identification of its central star

M. Santander-García, P. Rodríguez-Gil, O. Hernandez +9

The link between the shaping of bipolar planetary nebulae and their central stars is still poorly understood. The kinematics and shaping of the multipolar nebula M 1-75 are hereby…