dor_id: 51592

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336.#.#.b: article

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336.#.#.a: Artículo

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856.4.0.u: http://www.revistas.unam.mx/index.php/revmexaa/article/view/31410/29740

100.1.#.a: López, J. A.; Richer, M. G.; García-díaz, M. T.; Clark, D. M.; Meaburn, J.; Riesgo, H.; Steffen, W.; Lloyd, M.; López, J. A.; Richer, M. G.; García-díaz, M. T.; Clark, D. M.; Meaburn, J.; Riesgo, H.; Steffen, W.; Lloyd, M.

524.#.#.a: López, J. A., et al. (2012). The San Pedro Mártir Kinematic Catalogue of Galactic Planetary Nebulae. Revista Mexicana de Astronomía y Astrofísica; Vol 48, No 1, 2012; 3-7. Recuperado de https://repositorio.unam.mx/contenidos/51592

245.1.0.a: The San Pedro Mártir Kinematic Catalogue of Galactic Planetary Nebulae

502.#.#.c: Universidad Nacional Autónoma de México

561.1.#.a: Instituto de Astronomía, UNAM

264.#.0.c: 2012

264.#.1.c: 2012-04-24

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001.#.#.#: oai:ojs.phoenicis.tic.unam.mx:article/31410

041.#.7.h: eng

520.3.#.a: The San Pedro Mártir kinematic catalogue of galactic planetary nebulae provides spatially resolved, long-slit, Echelle spectra for about 600 planetary nebulae. The data are presented wavelength calibrated and corrected for heliocentric motion. For most objects multiple spectra have been acquired and images with accurate slit positions on the nebula are also presented for each object. This is the most extensive and homogeneous single source of data concerning the internal kinematics of the ionized nebular material in planetary nebulae. Data can be retrieved for individual objects or selected by groups that share some common characteristic, such as by morphological classes, galactic population, binary cores, presence of fast outflows, etc. The catalogue is available through the world wide web at http://kincatpn.astrosen.unam.mx.The San Pedro Mártir kinematic catalogue of galactic planetary nebulae provides spatially resolved, long-slit, Echelle spectra for about 600 planetary nebulae. The data are presented wavelength calibrated and corrected for heliocentric motion. For most objects multiple spectra have been acquired and images with accurate slit positions on the nebula are also presented for each object. This is the most extensive and homogeneous single source of data concerning the internal kinematics of the ionized nebular material in planetary nebulae. Data can be retrieved for individual objects or selected by groups that share some common characteristic, such as by morphological classes, galactic population, binary cores, presence of fast outflows, etc. The catalogue is available through the world wide web at http://kincatpn.astrosen.unam.mx.

773.1.#.t: Revista Mexicana de Astronomía y Astrofísica; Vol 48, No 1 (2012); 3-7

773.1.#.o: http://www.revistas.unam.mx/index.php/revmexaa/index

046.#.#.j: 2021-08-03 00:00:00.000000

022.#.#.a: ISSN impreso: 0185-1101

310.#.#.a: Semestral

300.#.#.a: Páginas: 3-7

264.#.1.b: Instituto de Astronomía, UNAM

758.#.#.1: http://www.revistas.unam.mx/index.php/revmexaa/index

handle: 15104aa54d800675

harvesting_date: 2019-02-06 00:00:00.0

856.#.0.q: application/pdf

245.1.0.b: The San Pedro Mártir Kinematic Catalogue of Galactic Planetary Nebulae

last_modified: 2021-08-12 16:00:00

license_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode.es

license_type: by-nc-nd

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No entro en nada

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Artículo

The San Pedro Mártir Kinematic Catalogue of Galactic Planetary Nebulae

López, J. A.; Richer, M. G.; García-díaz, M. T.; Clark, D. M.; Meaburn, J.; Riesgo, H.; Steffen, W.; Lloyd, M.; López, J. A.; Richer, M. G.; García-díaz, M. T.; Clark, D. M.; Meaburn, J.; Riesgo, H.; Steffen, W.; Lloyd, M.

Instituto de Astronomía, UNAM, publicado en Revista Mexicana de Astronomía y Astrofísica, y cosechado de Revistas UNAM

Licencia de uso

Procedencia del contenido

Cita

López, J. A., et al. (2012). The San Pedro Mártir Kinematic Catalogue of Galactic Planetary Nebulae. Revista Mexicana de Astronomía y Astrofísica; Vol 48, No 1, 2012; 3-7. Recuperado de https://repositorio.unam.mx/contenidos/51592

Descripción del recurso

Autor(es)
López, J. A.; Richer, M. G.; García-díaz, M. T.; Clark, D. M.; Meaburn, J.; Riesgo, H.; Steffen, W.; Lloyd, M.; López, J. A.; Richer, M. G.; García-díaz, M. T.; Clark, D. M.; Meaburn, J.; Riesgo, H.; Steffen, W.; Lloyd, M.
Tipo
Artículo de Investigación
Área del conocimiento
Físico Matemáticas y Ciencias de la Tierra
Título
The San Pedro Mártir Kinematic Catalogue of Galactic Planetary Nebulae
Fecha
2012-04-24
Resumen
The San Pedro Mártir kinematic catalogue of galactic planetary nebulae provides spatially resolved, long-slit, Echelle spectra for about 600 planetary nebulae. The data are presented wavelength calibrated and corrected for heliocentric motion. For most objects multiple spectra have been acquired and images with accurate slit positions on the nebula are also presented for each object. This is the most extensive and homogeneous single source of data concerning the internal kinematics of the ionized nebular material in planetary nebulae. Data can be retrieved for individual objects or selected by groups that share some common characteristic, such as by morphological classes, galactic population, binary cores, presence of fast outflows, etc. The catalogue is available through the world wide web at http://kincatpn.astrosen.unam.mx.The San Pedro Mártir kinematic catalogue of galactic planetary nebulae provides spatially resolved, long-slit, Echelle spectra for about 600 planetary nebulae. The data are presented wavelength calibrated and corrected for heliocentric motion. For most objects multiple spectra have been acquired and images with accurate slit positions on the nebula are also presented for each object. This is the most extensive and homogeneous single source of data concerning the internal kinematics of the ionized nebular material in planetary nebulae. Data can be retrieved for individual objects or selected by groups that share some common characteristic, such as by morphological classes, galactic population, binary cores, presence of fast outflows, etc. The catalogue is available through the world wide web at http://kincatpn.astrosen.unam.mx.
Idioma
eng
ISSN
ISSN impreso: 0185-1101

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