Volume 529, May 2011
|Number of page(s)||6|
|Section||Interstellar and circumstellar matter|
|Published online||06 April 2011|
Improved prospects for the detection of new Large Magellanic Cloud planetary nebulae⋆
Centre for Astrophysics Research, STRI, University of Hertfordshire, College Lane Campus, Hatfield AL10 9AB, UK
2 University Observatory Munich, Scheinerstrasse 1, 81679 München, Germany
3 Research School of Astronomy and Astrophysics, Australian National University, Cotter Road, Weston Creek ACT 2611, Australia
4 Department of Astronomy, Beijing Normal University, Beijing 100875, PR China
Received: 3 December 2010
Accepted: 10 March 2011
The Large Magellanic Cloud (LMC) contains the nearest large extragalactic population of planetary nebulae (PNe). A shallow viewing angle and low interstellar reddening towards the LMC potentially means a larger, more complete flux-limited population can be assembled than for any other galaxy. These advantages appear to be reflected by the small gap between the catalogued (~700 PNe) and estimated (1000 ± 250 PNe) population size. With more detailed multi-wavelength studies the catalogued number of LMC PNe may fall, potentially widening this gap. We demonstrate here that the gap can be further bridged with improved optical and near-infrared imaging surveys. We present three [O III]-selected PNe discovered from ESO WFI observations of the 30 Doradus region and one serendipitous discovery from near-infrared Vista Magellanic Cloud (VMC) survey observations. The WFI PNe have resolved [O III] and Hα nebulae that verify their PN nature and their [O III] fluxes place them 6–7 mag (m5007 = 20–21 mag) fainter than the bright-end of the planetary nebula luminosity function (PNLF). Their faintness, small angular size and surrounding complex emission-line background explains why previous surveys of the region did not select them. We estimate there may be as many as 50–75 similar PNe awaiting discovery in the central 5 × 5 degrees of the LMC. The VMC survey routinely detects PNe as resolved nebulae that may allow some of this expected population to be recovered without traditional narrow-band imaging surveys. We demonstrate this potential with the first new VMC-selected PN which has a rare Wolf-Rayet [WC9]–[WC11] central star.
Key words: planetary nebulae: general / Magellanic Clouds
Based on observations made with the Wide Field Imager of the Max-Planck-ESO 2.2 m telescope at La Silla Observatory under program ID 076.C-0888, processed and released by the ESO VOS/ADP group, VISTA at Paranal Observatory under program ID 179.B-2003 and the Wide Field Spectrograph of the Australian National University 2.3 m telescope.
© ESO, 2011
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