Bibcode
Viironen, K.; Greimel, R.; Corradi, R. L. M.; Mampaso, A.; Rodríguez, M.; Sabin, L.; Delgado-Inglada, G.; Drew, J. E.; Giammanco, C.; González-Solares, E. A.; Irwin, M. J.; Miszalski, B.; Parker, Q. A.; Rodríguez-Flores, E. R.; Zijlstra, A.
Referencia bibliográfica
Astronomy and Astrophysics, Volume 504, Issue 1, 2009, pp.291-301
Fecha de publicación:
9
2009
Revista
Número de citas
67
Número de citas referidas
57
Descripción
Context: We have carried out a semi-automated search for planetary
nebulae (PNe) in the INT photometric H-alpha survey (IPHAS) catalogue.
We present the PN search and the list of selected candidates. We cross
correlate the selected candidates with a number of existing infrared
galactic surveys in order to gain further insight into the nature of the
candidates. Spectroscopy of a subset of objects is used to estimate the
number of PNe present in the entire candidate list. Aims: The
overall aim of the IPHAS PN project is to carry out a deep census of PNe
in the northern Galactic plane, an area where PN detections are clearly
lacking. Methods: The PN search is carried out on the IPHAS
photometric catalogue. The candidate selection is based on the IPHAS and
2MASS/UKIDSS colours of the objects and the final candidate selection is
made visually. Results: From the original list of ~600 million
IPHAS detections we have selected a total of 1005 objects. Of these, 224
are known objects, leaving us with 781 PN candidates. Based on the
initial follow-up spectroscopy, we expect the list to include very young
and proto-PNe in addition to genuine, normal PNe (~16%) and emission
line objects other than PNe. We present additional criteria to select
the most probable PN candidates from our candidate list.
Table 1 is only available in electronic form at the CDS via anonymous
ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via
http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/504/291
Proyectos relacionados
Nebulosas Bipolares
Nuestro proyecto persigue tres objetivos principales: 1) Determinar las condiciones físico-químicas de las nebulosas planetarias con geometría bipolar y de las nebulosas alrededor de estrellas simbióticas. El fin es entender el origen de la bipolaridad y poner a prueba los modelos teóricos que intentan explicar la morfología y la cinemática nebular
Antonio
Mampaso Recio