A PILE OF NEW PLANETARY NEBULAE IN THE GALACTIC PLANE

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1. Verfasser: A. Mampaso
Format: Artículo científico
Sprache:en
Veröffentlicht: Universidad Nacional Autónoma de México 2009
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author A. Mampaso
author_facet A. Mampaso
contents A PILE OF NEW PLANETARY NEBULAE IN THE GALACTIC PLANE A. Mampaso R. L. M. Corradi K. Viironen L. Sabin IPHAS collaboratio Física, Astronomía y Matemáticas surveys stars: pre main sequence stars: mass loss Planetary nebulae: general The INT photometric H-alpha Survey (IPHAS; http://www.iphas.org) is now near completion. A band of 10 degrees along the Northern Galactic Plane is being imaged in H , r' and i' lters with typically 1 arcsec resolution and a completeness limit better than r'=20 mag. IPHAS is lling in the currently existing gap in the Planetary Nebulae (PNe) population of the Plane: we are on course to tripling the number of PNe known in the northern plane. Many hundreds of candidate PNe, both small diameter (<10 arcsec) and extended, have been identied; some are located in areas of particular interest as the Anticenter region. A preliminary analysis of the region from RA=18 to 20h, where the observations are already complete, is presented. 2009 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57115758039 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.35
format Artículo científico
id redalyc_57115758039
institution Redalyc
language en
publishDate 2009
publisher Universidad Nacional Autónoma de México
spellingShingle A PILE OF NEW PLANETARY NEBULAE IN THE GALACTIC PLANE
A. Mampaso
Física, Astronomía y Matemáticas
surveys
stars: pre
main sequence
stars: mass loss
Planetary nebulae: general
A PILE OF NEW PLANETARY NEBULAE IN THE GALACTIC PLANE A. Mampaso R. L. M. Corradi K. Viironen L. Sabin IPHAS collaboratio Física, Astronomía y Matemáticas surveys stars: pre main sequence stars: mass loss Planetary nebulae: general The INT photometric H-alpha Survey (IPHAS; http://www.iphas.org) is now near completion. A band of 10 degrees along the Northern Galactic Plane is being imaged in H , r' and i' lters with typically 1 arcsec resolution and a completeness limit better than r'=20 mag. IPHAS is lling in the currently existing gap in the Planetary Nebulae (PNe) population of the Plane: we are on course to tripling the number of PNe known in the northern plane. Many hundreds of candidate PNe, both small diameter (<10 arcsec) and extended, have been identied; some are located in areas of particular interest as the Anticenter region. A preliminary analysis of the region from RA=18 to 20h, where the observations are already complete, is presented. 2009 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57115758039 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.35
title A PILE OF NEW PLANETARY NEBULAE IN THE GALACTIC PLANE
topic Física, Astronomía y Matemáticas
surveys
stars: pre
main sequence
stars: mass loss
Planetary nebulae: general
url https://www.redalyc.org/articulo.oa?id=57115758039