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Authors: Saito, R. K | Hempel, M | Hodgkin, S. T | Stead, J | Stephens, A. W | Tamura, M | Tappert, C | Thompson, M. A | Valenti, E | Vanzi, L | Walton, N. A | Weidmann, W | Zijlstra, A | Lewis, J. R | Cross, N | Ivanov, V. D | Kerins, E | Emerson, J. P | Soto, M | Amôres, E. B | Gurovich, S | Dékány, I | Minniti, D | Angeloni, R | Beamin, J. C | Catelan, M | Padilla, N | Zoccali, M | Pietrukowicz, P | Moni Bidin, C | Mauro, F | Geisler, D | Folkes, S. L | Lucas, P. W | Sale, S. E | Borissova, J | Kurtev, R | Ahumada, A. V | Alonso, M. V | Adamson, A | Arias, J. I | Bandyopadhyay, R. M | Barbá, R. H | Barbuy, B | Rejkuba, M | Baume, G. L | Bedin, L. R | Bellini, A | Benjamin, R | Bica, E | Bonatto, C | Bronfman, L | Carraro, G | Chene, A. N | Clariá, J. J | Toledo, I | Clarke, J. R. A | Contreras, C | Corvillón, A | de Grijs, R | Dias, B | Drew, J. E | Fariña, C | Feinstein, C | Fernández-Lajús, E | Gamen, R. C | Gonzalez, O. A | Gieren, W | Goldman, B | González-Fernández, C | Grand, R. J. J | Gunthardt, G | Hambly, N. C | Hanson, M. M | Helminiak, K. G | Hoare, M. G | Huckvale, L | Alonso-García, J | Jordán, A | Kinemuchi, K | Longmore, A | López-Corredoira, M | MacCarone, T | Majaess, D | Martín, E. L | Masetti, N | Mennickent, R. E | Mirabel, I. F | Irwin, M. J | Monaco, L | Morelli, L | Motta, V | Palma, T | Parisi, M. C | Parker, Q | Peñaloza, F | Pietrzyński, G | Pignata, G | Popescu, B | Gonzalez-Solares, E | Read, M. A | Rojas, A | Roman-Lopes, A | Ruiz, M. T | Saviane, I | Schreiber, M. R | Schröder, A. C | Sharma, S | Smith, M. D | Sodré Jr., L
Date: 2012
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/177433
Description: 21 page(s)
Reviewed:Reviewed
Date: 2011
Subject Keyword: Galaxy: abundances
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/158292
Description: Aims. A proper determination of the abundance gradient in the Milky Way requires the observation of objects at large galactiocentric distances. With this aim, we are exploring the planetary nebula pop... More
Reviewed:Reviewed
Date: 2011
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/156776
Description: 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-1, and a fast collimated outflow in the f... More
Reviewed:Reviewed
Date: 2010
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/133194
Description: Context. Knowledge of the total population of symbiotic stars in the Galaxy is important for understanding basic aspects of stellar evolution in interacting binaries and the relevance of this class of... More
Reviewed:Reviewed
Date: 2009
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/88348
Description: Aims. We search for very small-diameter galactic planetary nebulae (PNe) representing the earliest phases of PN evolution. The IPHAS catalogue of Hα-emitting stars provides a useful basis for this stu... More
Full Text: Full Text
Reviewed:Reviewed
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