The UV-Excess survey of the northern Galactic plane

Bibcode
2009MNRAS.399..323G
DOI
10.1111/j.1365-2966.2009.15273.x
Groot, Paul J.; Verbeek, Kars; Greimel, Robert; Irwin, Mike; González-Solares, Eduardo; Gänsicke, Boris T.; de Groot, Eelco; Drew, Janet; Augusteijn, Thomas; Aungwerojwit, Amornrat; Barlow, Mike; Barros, Susana; van den Besselaar, Else J. M.; Casares, Jorge; Corradi, Romano; Corral-Santana, Jesús M.; Deacon, Niall; van Ham, Wilbert; Hu, Haili; Heber, Uli; Jonker, Peter G.; King, Rob; Knigge, Christian; Mampaso, Antonio; Marsh, Tom R.; Morales-Rueda, Luisa; Napiwotzki, Ralf; Naylor, Tim; Nelemans, Gijs; Oosting, Tim; Pyrzas, Stylianos; Pretorius, Magaretha; Rodríguez-Gil, Pablo; Roelofs, Gijs H. A.; Sale, Stuart; Schellart, Pim; Steeghs, Danny; Szyszka, Cezary; Unruh, Yvonne; Walton, Nicholas A.; Weston, Simon; Witham, Andrew; Woudt, Patrick; Zijlstra, Albert
Bibliographical reference

Monthly Notices of the Royal Astronomical Society, Volume 399, Issue 1, pp. 323-339.

Advertised on:
10
2009
Journal
Monthly Notices of the Royal Astronomical Society
Number of authors
44
IAC number of authors
5
Citations
64
Refereed citations
56
Description
The UV-Excess survey of the northern Galactic plane images a 10° × 185° wide band, centred on the Galactic equator using the 2.5-m Isaac Newton Telescope in four bands (I5875) down to ~21-22 mag ( in I5875). The setup and data reduction procedures are described. Simulations of the colours of main-sequence stars, giant, supergiants, DA and DB white dwarfs and AM Canum Venaticorum stars are made, including the effects of reddening. A first look at the data of the survey (currently 30 per cent complete) is given.
Related projects
Planetary Nebula "The Necklace"
Bipolar Nebulae
This project has three major objectives: 1) To determine the physico-chemical characteristics of bipolar planetary nebulae and symbiotic nebulae, to help understanding the origin of bipolarity and to test theoretical models, mainly models with binary central stars, aimed at explaining the observed morphology and kinematics. 2) To study the low
Antonio
Mampaso Recio
Closed
Representación de la variable cataclísmica SS Cygni (Chris Moran)
Binary Stars
The study of binary stars is essential to stellar astrophysics. A large number of stars form and evolve within binary systems. Therefore, their study is fundamental to understand stellar and galactic evolution. Particularly relevant is that binary systems are still the best source of precise stellar mass and radius measurements. Research lines
Pablo
Rodríguez Gil
In progress
Type
Refereed
Stellar & Interstellar Physics (FEEI)
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