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相关论文: Planetary Nebula NGC 2818: Revealing its complex 3…

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High-resolution Hubble Space Telescope (HST) archive imaging and high-dispersion spectroscopy are used to study the complex morphological and kinematical structure of the planetary nebula, NGC 2818. We analyze narrow band H{\alpha}, [O…

太阳与恒星天体物理 · 物理学 2015-06-04 Roberto Vázquez

We present the kinematics of a sample of bipolar planetary nebulae (PNe) which cover a wide range of observed morphologies and collimation degrees, from bipolar PNe with a marked equatorial ring and wide lobes to highly collimated objects.…

天体物理学 · 物理学 2009-11-13 Martina Dobrincic , Eva Villaver , Martin A. Guerrero , Arturo Manchado

In search for deviations from homologous expansion in planetary nebulae we present a 3D morphokinematical model of NGC 7009. The model has been constructed with {\em Shape} based on PV diagrams from the literature and HST images. We find…

太阳与恒星天体物理 · 物理学 2009-05-14 W. Steffen , M. Espindola , S. Martinez , N. Koning

In this paper we present the results of optical high-resolution imaging and spectroscopy of the complex planetary nebula (PN) NGC~3242. Our study is based on the analysis of the narrowband H$\alpha$ $\lambda$6563\AA , [O III]…

太阳与恒星天体物理 · 物理学 2015-09-30 M. A. Gómez-Muñoz , M. W. Blanco Cárdenas , R. Vázquez , S. Zavala , P. F. Guillén , S. Ayala

Aims. Numerous planetary nebulae show complicated inner structures not obviously explained. For one such object we undertake a detailed 3D photoionization and kinematical model analysis for a better understanding of the underlying shaping…

太阳与恒星天体物理 · 物理学 2024-08-28 K. Gesicki , A. Zijlstra , M. Hajduk , A. Iwanowska , K. Grzesiak , K. Lisiecki , J. Lipinski

The kinematics of the bipolar planetary nebulae Hb~5 and K 3-17 are investigated in detail by means of a comprehensive set of spatially resolved high spectral resolution, long-slit spectra. Both objects share particularly interesting…

星系天体物理 · 物理学 2015-06-04 J. A. López , Ma. T. García-Díaz , W. Steffen , H. Riesgo , M. G. Richer

We have studied the planetary nebula (PN) NGC 6572 through 3D morpho-kinematic and photoionization modelling. The 3D morphology is reconstructed from the Hubble Space Telescope images in different narrow band filters and position-velocity…

太阳与恒星天体物理 · 物理学 2023-07-05 Rahul Bandyopadhyay , Ramkrishna Das , Mudumba Parthasarathy , Subhajit Kar

We present high-resolution, long-slit spectroscopic observations of five compact ($\leq$ 10 arcsec) planetary nebulae located close to the galactic bulge region and for which no high spatial resolution images are available. The data have…

太阳与恒星天体物理 · 物理学 2015-06-05 S. Akras , J. A. López

We present an extensive, long-slit, high-resolution coverage of the complex planetary nebula (PN), NGC 7026. We acquired ten spectra using the Manchester Echelle Spectrometer at San Pedro Martir Observatory in Baja California, Mexico, and…

星系天体物理 · 物理学 2015-06-11 D. M. Clark , J. A. López , W. Steffen , M. G. Richer

We present a new modeling tool for planetary nebulae (PNe), based on 3D photoionization calculations. From models for two theoretical PNe, we show that the enhancement in the equatorial zone observed in several PNe is not necessarily due to…

天体物理学 · 物理学 2007-05-23 H. Monteiro , C. Morisset , R. Gruenwald , S. M. Viegas

This work describes the modelling of the 3D structure and position-velocity (P-V) diagrams of NGC 2440, a well known planetary nebula, aiming to describe the morphology of this object, specially its core. We have used high resolution…

太阳与恒星天体物理 · 物理学 2016-06-06 Paulo J. A. Lago , Roberto D. D. Costa

We present a new modeling tool for planetary nebulae, based on 3D photoionization calculations. Our goal is to show that all the information provided by observations, regarding kinematics and morphology, have to be consistently accounted…

天体物理学 · 物理学 2009-10-31 C. Morisset , R. Gruenwald , S. M. Viegas

We analyze optical images and high-resolution, long-slit spectra of three planetary nebulae which possess collimated, low-ionization features. NGC 3918 is composed of an inner, spindle-shaped shell mildly inclined with respect to the plane…

天体物理学 · 物理学 2009-10-31 Romano L. M. Corradi , Mario Perinotto , Eva Villaver , Antonio Mampaso , Denise R. Goncalves

We present the first part of an investigation on the planetary nebula (PN) PC 22 which focuses on the use of deep imaging and high resolution echelle spectroscopy to perform a detailed morpho-kinematical analysis. PC 22 is revealed to be a…

We present a detailed kinematical analysis of the young compact hourglass-shaped planetary nebula Hb 12. We performed optical imaging and longslit spectroscopy of Hb 12 using the Manchester echelle spectrometer with the 2.1m San Pedro…

星系天体物理 · 物理学 2015-05-13 N. M. H. Vaytet , A. P. Rushton , M. Lloyd , J. A. López , J. Meaburn , T. J. O'Brien , D. L. Mitchell , D. Pollacco

We present new narrow-band Ha, [N II], and [O III] high-resolution images of the quadrupolar planetary nebula (PN) NGC 6309 that show in great detail its bipolar lobes and reveal new morphological features. New high- and low-dispersion…

太阳与恒星天体物理 · 物理学 2015-06-23 Gabriel Rubio , Roberto Vazquez , Gerardo Ramos-Larios , Martin A. Guerrero , Lorenzo Olguin , Pedro F. Guillen , Hector Mata

We present a set of optical and infrared images combined with long-slit, medium and high dispersion spectra of the southern planetary nebula (PN) NGC 5189. The complex morphology of this PN is puzzling and has not been studied in detail so…

太阳与恒星天体物理 · 物理学 2012-03-07 L. Sabin , R. Vázquez , J. A. López , Ma. T. García-Díaz , G. Ramos-Larios

Planetary nebulae (PNe) that are physical members of open star clusters (OCs) are valuable for stellar evolution studies. They are extremely rare, with only three such instances confirmed in our Galaxy. Here, we confirm the physical…

太阳与恒星天体物理 · 物理学 2025-03-26 Vasiliki Fragkou , Roberto Vázquez , Quentin A. Parker , Denise R. Gonçalves , Luis Lomelí-Núñez

We present the first detailed spatio-kinematical analysis and modelling of the Southern planetary nebula SuWt 2. This object presents a problem for current theories of planetary nebula formation and evolution, as it is not known to contain…

太阳与恒星天体物理 · 物理学 2011-11-18 D. Jones , M. Lloyd , D. L. Mitchell , D. L. Pollacco , T. J. O'Brien , N. M. H. Vaytet

We use a 3D photoionization modeling tool to study the morpho-kinematic properties of the Planetary Nebula (PN) NGC 3132. We show that it is possible to reproduce the low resolution observations (spectra and images) with an ellipsoidal…

天体物理学 · 物理学 2009-10-31 H. Monteiro , C. Morisset , R. Gruenwald , S. M. Viegas
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