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相关论文: Multiple Point-Symmetric Ejections in IC 4634

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With its remarkable double-S shape, IC 4634 is an archetype of point-symmetric planetary nebulae (PN). In this paper, we present a detailed study of this PN using archival HST WFPC2 and ground-based narrow-band images to investigate its…

天体物理学 · 物理学 2009-11-13 M. A. Guerrero , L. F. Miranda , A. Riera , P. F. Velazquez , L. Olguin , R. Vazquez , Y. -H. Chu , A. Raga , G. Benitez

We present images and high-resolution spectra of the planetary nebulae IC 2553 and NGC 5882. Spatio-kinematic modeling of the nebulae shows that they are composed of a markedly elongated inner shell, and of a less aspherical outer shell…

天体物理学 · 物理学 2009-10-31 R. L. M. Corradi , D. R. Goncalves , E. Villaver , A. Mampaso , M. Perinotto

We have obtained narrow-band images and high-resolution spectra of the planetary nebulae NGC 6337, He 2-186, and K 4-47, with the aim of investigating the relation between their main morphological components and several low-ionization…

We report the detection of near-IR H$_2$ emission from the low-ionization structures (knots) in two planetary nebulae. The deepest ever, high-angular resolution H$_2$ 1-0 S(1) at 2.122$\mu$, H$_2$ 2-1 S(1) at 2.248$\mu$ and Br$\gamma$…

太阳与恒星天体物理 · 物理学 2016-12-21 Stavros Akras , Denise R. Gonçalves , Gerardo Ramos-Larios

In this 5th paper of the series, we examine the spectroscopy and morphology of four southern Galactic planetary nebulae Hen 2-141, NGC5307, IC 2553, and PB6 using new integral field spectroscopy data. The morphologies and ionization…

太阳与恒星天体物理 · 物理学 2017-11-08 A. Ali , M. A. Dopita

K 4-47 is an unusual planetary nebula composed of a compact high-ionization core and a pair of low-ionization knots. Long-slit medium-resolution spectra of the knots and core are analyzed in this paper. Assuming photoionization from the…

天体物理学 · 物理学 2009-11-10 D. R. Goncalves , A. Mampaso , R. L. M. Corradi , M. Perinotto , A. Riera , L. Lopez-Martin

We present the analysis of Very Large Telescope (VLT) Multi Unit Spectroscopic Explorer (MUSE) observations of the planetary nebula (PN) IC 4406. MUSE images in key emission lines are used to unveil the presence of at least 5 ring-like…

太阳与恒星天体物理 · 物理学 2022-03-14 G. Ramos-Larios , J. A. Toalá , J. B. Rodríguez-González , M. A. Guerrero , V. M. A. Gómez-González

We present narrow-band images and long-slit echelle spectra of the planetary nebula (PN) NGC 6778. The data show this PN as bipolar, with a very prominent low-excitation equatorial toroid, high-excitation lobes and two pairs of collimated…

天体物理学 · 物理学 2007-05-23 Vicente Maestro , Martin A. Guerrero , Luis F. Miranda

In order to assess qualitatively the ejecta geometry of stripped-envelope core-collapse supernovae, we investigate 98 late-time spectra of 39 objects, many of them previously unpublished. We perform a Gauss-fitting of the [O I] 6300, 6364…

The optical line and continuum emission in the very high ionization Galactic planetary nebula (PN) NGC 4361 (PN G294.1 +43.6), has been mapped with VLT MUSE Wide Field normal mode (4750-9300A) commissioning observations. The PN is larger…

太阳与恒星天体物理 · 物理学 2024-10-16 J. R. Walsh , A. Monreal Ibero , J. Laging , M. Romeijnders

We present the analysis of the planetary nebula (PN) NGC 2371 around the [Wolf-Rayet] ([WR]) star WD 0722$+$295. Our Isaac Newton Telescope (INT) Intermediate Dispersion Spectrograph (IDS) spectra, in conjunction with archival optical and…

太阳与恒星天体物理 · 物理学 2020-06-10 V. M. A. Gómez-González , J. A. Toalá , M. A. Guerrero , H. Todt , L. Sabin , G. Ramos-Larios , Y. D. Mayya

The jets seen in NGC 6543 motivated us to search for similar features in other PNe. Our HST snapshot program looked for jets using the [N II] and H-alpha narrow-band filters. Although spectacular jets are found in proto-PNe, true jets seem…

天体物理学 · 物理学 2007-05-23 J. Patrick Harrington , Kazimierz J. Borkowski

We have studied the nearby old pulsar PSR B1929+10 and its surrounding interstellar medium utilizing the sub-arcsecond angular resolution of the Chandra X-ray Observatory. The Chandra data are found to be fully consistent with the results…

天体物理学 · 物理学 2009-11-13 C. Y. Hui , W. Becker

We present spectra and high resolution images of the hard X-ray feature along the southern edge of the supernova remnant IC443. Data from the Chandra X-ray Observatory reveal a comet-shaped nebula of hard emission, which contains a softer…

天体物理学 · 物理学 2009-11-06 C. M. Olbert , C. R. Clearfield , N. E. Williams , J. W. Keohane , D. A. Frail

We report near-infrared integral field spectroscopic observations of the active galactic nucleus NGC 4151 with archive data from the NIFS-Gemini North Telescope. We have selected best-seeing observations ($\lesssim$0.3 arcsec) that, allied…

星系天体物理 · 物理学 2020-07-16 D. May , J. E. Steiner , R. B. Menezes , D. R. A. Williams , J. Wang

We find that a non-axisymmetric bow shock model, with an appropriate choice of parameters, could fit the line splitting velocity field of the cone-like H$\alpha$ nebula in NGC 4945 better than a canonical cone model. Meanwhile, the bow…

天体物理学 · 物理学 2016-08-30 Yang Chen , Jie-Hao Huang

We present conspicuous activities of plasma ejections along a light bridge of a stable and mature sunspot in NOAA 8971 on 2000 May 02. We found the ejections both in the H-alpha (10^4 K) images obtained with the Domeless Solar Telescope…

天体物理学 · 物理学 2009-11-07 Ayumi Asai , Takako T. Ishii , Hiroki Kurokawa

The protostar IRAS 15398-3359 is associated with a bipolar molecular outflow ejected in an nearly northeast-southwest (NE-SW) direction which has been extensively studied. It has been suggested previous episodic accretion events by this…

太阳与恒星天体物理 · 物理学 2024-06-12 E. Guzmán Ccolque , M. Fernández López , M. M. Vazzano , I. de Gregorio , A. Plunkett , A. Santamaría-Miranda

We present a detailed analysis of IC 4776, a planetary nebula displaying a morphology believed to be typical of central star binarity. The nebula is shown to comprise a compact hourglass-shaped central region and a pair of precessing…

We present new NICMOS/HST infrared images and CGS4/UKIRT Br-alpha (4.05 um) spectroscopy of the Pistol Star and its associated nebula, finding strong evidence to support the hypothesis that the Pistol Nebula was ejected from the Pistol…

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