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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

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

The WFPC2 camera aboard the HST was used to obtain images of the planetary nebula BD+30 3639 at two epochs separated by 5.663 years. The expansion of the nebula in the H-alpha and [N II] bands has been measured using several methods.…

天体物理学 · 物理学 2009-11-07 Jianyang Li , J. Patrick Harrington , Kazimierz J. Borkowski

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

We present high quality radio continuum observations made with the Very Large Array (VLA) at 3.6 cm at two epochs toward the planetary nebula M2-43. The comparison of the two epochs, obtained with a time separation of 4.07 years, clearly…

天体物理学 · 物理学 2007-05-23 L. Guzman , Y. Gomez , L. F. Rodriguez

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 high-dispersion echelle spectroscopic observations and a narrow-band [N II] image of the remarkable jet-like features of He 2-90. They are detected in the echelle spectra in the H-alpha and [N II] lines but not in other nebular…

天体物理学 · 物理学 2009-11-07 Martin A. Guerrero , Luis F. Miranda , You-Hua Chu , Monica Rodriguez , Rosa M. Williams

We present narrow-band optical and near-IR imaging and optical long-slit spectroscopic observations of Hu1-2, a Galactic planetary nebula (PN) with a pair of [N II]-bright, fast-moving (> 340 km/s) bipolar knots. Intermediate-dispersion…

太阳与恒星天体物理 · 物理学 2015-08-06 Xuan Fang , Martin A. Guerrero , Luis F. Miranda , Angels Riera , Pablo F. Velazquez , Alejandro C. Raga

We present the analysis of several newly obtained and archived photometric and spectroscopic datasets of the intriguing and yet poorly understood 13.5-mag central star candidate of the bipolar planetary nebula Sh2-71. Photometric…

太阳与恒星天体物理 · 物理学 2015-05-08 Teo Močnik , Myfanwy Lloyd , Don Pollacco , Rachel A. Street

We present high-dispersion spectroscopic data of the compact planetary nebula Vy 1-2, where high expansion velocities up to 100 km/s are found in the Ha, [N II] and [O III] emission lines. HST images reveal a bipolar structure. Vy 1-2…

太阳与恒星天体物理 · 物理学 2016-08-08 S. Akras , P. Boumis , J. Meaburn , J. Alikakos , J. A. López , D. R. Gonçalves

We present a comprehensive set of spatially resolved, integral field spectroscopic mapping of the Wolf-Rayet planetary nebula Th 2-A, obtained using the Wide Field Spectrograph on the Australian National University 2.3-m telescope.…

太阳与恒星天体物理 · 物理学 2015-12-09 Ashkbiz Danehkar

We apply an axially symmetric pseudo-3D photoionization model, pyCloudy, to derive the structures of 6 bipolar nebulae and 2 suggested post-bipolars in a quest to constrain the bipolar planetary nebulae evolution. HST images and VLT/UVES…

太阳与恒星天体物理 · 物理学 2015-12-22 K. Gesicki , A. A. Zijlstra , C. Morisset

The catalogue of protoplanetary nebulae by Vickers et al. has been supplemented with the line-of-sight velocities and proper motions of their central stars from the literature. Based on an exponential density distribution, we have estimated…

星系天体物理 · 物理学 2017-06-01 V. V. Bobylev , A. T. Bajkova

We present high-dispersion long-slit IR spectra of the double-shell bipolar planetary nebula M 2-9 in the emission lines [Fe II] 16435 and H2 v=1--0 S(1) 21218. H2 spectra reveal for the first time the kinematic structure of the outer shell…

天体物理学 · 物理学 2009-09-29 Nathan Smith , Bruce Balick , Robert D. Gehrz

We present near-IR narrow-band continuum-subtracted images in the H$_2$ $2.122\mu$m, and Br$\gamma$ $2.166\mu$m emission lines for a sample of 15 bipolar planetary nebulae. H$_2$ emission was definitely detected for most of the objects in…

天体物理学 · 物理学 2009-10-31 M. A. Guerrero , E. Villaver , A. Manchado , P. Garcia-Lario , F. Prada

Hu\,1-2 is a planetary nebula that contains an isolated knot located northwestern of the main nebula, which could be related to a collimated outflow. We present a subsarcsecond H$\alpha$+[N\,{\sc ii}] image and a high-resolution, long-slit…

星系天体物理 · 物理学 2015-06-03 L. F. Miranda , M. Blanco , M. A. Guerrero , A. Riera

The object of this study is one of the most energetic and luminous molecular outflows known in the Galaxy, G331.512-0.103. Observations with ALMA Band 7 (350 GHz; 0.86 mm) reveal a very compact, extremely young bipolar outflow and a more…

We present low and high resolution long-slit spectra of three bipolar planetary nebulae (PNe) with bright central cores: A79, He2-428 and M1-91. He2-428 and M1-91 have high density (from 10^3.3 to 10^6.5 cm^-3) unresolved nebular cores that…

天体物理学 · 物理学 2009-11-07 M. Rodriguez , R. L. M. Corradi , A. Mampaso

We analyse the point-symmetric planetary nebula NGC 6309 in terms of its three-dimensional structure and of internal variations of the physical conditions to deduce the physical processes involved in its formation. We used VLA-D 3.6-cm…

天体物理学 · 物理学 2009-11-13 R. Vázquez , L. F. Miranda , L. Olguín , S. Ayala , J. M. Torrelles , M. E. Contreras , P. F. Guillén

The kinematics and physical conditions of the bipolar planetary nebula M 2-48 are analysed from high and low dispersion long-slit spectra. Previous CCD narrow-band optical observations have suggested that this nebula is mainly formed by a…

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