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We investigate the morphology of the collision front between the stellar winds of binary components in two long-period binary systems, one consisting of a hydrogen rich Wolf-Rayet star (WNL) and an O-star and the other of a Luminous Blue…

星系天体物理 · 物理学 2011-05-13 Allard Jan van Marle , Rony Keppens , Zakaria Meliani

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

Our understanding of Pulsar Wind Nebulae (PWNe), has greatly improved in the last years thanks to unprecedented high resolution images taken from the HUBBLE, CHANDRA and XMM satellites. The discovery of complex but similar inner features,…

天体物理学 · 物理学 2009-06-23 N. Bucciantini

Radio continuum observations trace thermal emission of ionized plasma in planetary nebulae and bring useful information on nebular geometries. A model of homogeneous sphere or shell cannot fit the nebular spectra and brightness…

Studies of the relationship between planetary nebula morphology and the evolution of the central stars has long suffered from uncertainties in distance determinations, and from the bias of interstellar absorption, that are typical for…

天体物理学 · 物理学 2007-05-23 L. Stanghellini , R. A. Shaw , J. C. Blades , B. Balick

The dust cloud around $\lambda$ Orionis is observed to be circularly symmetric with a large angular extent ($\approx$ 8 degrees). However, whether the three-dimensional (3D) structure of the cloud is shell- or ring-like has not yet been…

星系天体物理 · 物理学 2015-05-25 Dukhang Lee , Kwang-Il Seon , Young-Soo Jo

The kinematic structure of a sample of planetary nebulae, consisting of 23 [WR] central stars, 21 weak emission line stars (wels) and 57 non-emission line central stars, is studied. The [WR] stars are shown to be surrounded by turbulent…

天体物理学 · 物理学 2009-11-11 K. Gesicki , A. A. Zijlstra , A. Acker , S. K. Gorny , K. Gozdziewski , J. R. Walsh

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 deep imaging from the Dark Energy Camera to explore the peripheral regions of nine globular clusters in the outer halo of the Milky Way. Apart from Whiting 1 and NGC 7492, which are projected against the Sagittarius stream, we see no…

星系天体物理 · 物理学 2022-03-30 Shumeng Zhang , Dougal Mackey , Gary Da Costa

We report the results from an optical imaging survey of proto-planetary nebula candidates using the HST. We exploited the high resolving power and wide dynamic range of HST and detected nebulosities in 21 of 27 sources. All detected…

天体物理学 · 物理学 2009-10-31 Toshiya Ueta , Margaret Meixner , Matthew Bobrowsky

We have carried out integral field unit (IFU) spectroscopy of H$\alpha$, [N II] and [O III] emission lines for a sample of Galactic planetary nebulae (PNe) with Wolf-Rayet (WR) stars and weak emission-line stars (wels). Comparing their…

太阳与恒星天体物理 · 物理学 2015-11-06 Ashkbiz Danehkar , Wolfgang Steffen , Quentin A. Parker

A spherical planetary nebula is described as a geometric model. The nebula itself is considered as a thin-shell which visualized as a boundary of two spacetimes. The inner and outer curvature tensors of the thin-shell are found in order to…

广义相对论与量子宇宙学 · 物理学 2020-10-20 S. Danial Forghani , Ibrahim Gullu , S. Habib Mazharimousavi

We present a multiwavelength study of the iconic Bubble Nebula (NGC 7635) and its ionising star BD$+$60$^{\circ}$2522. We obtained XMM-Newton EPIC X-ray observations to search for extended X-ray emission as in other similar wind-blown…

太阳与恒星天体物理 · 物理学 2020-04-29 J. A. Toalá , M. A. Guerrero , H. Todt , L. Sabin , L. M. Oskinova , Y. -H. Chu , G. Ramos-Larios , V. M. A. Gómez-González

We present images and light curves of the bipolar Planetary Nebula RPJ 053059-683542 that was discovered in the Reid-Parker AAO/UKST H-alpha survey of the Large Magellanic Cloud (LMC). The emission from this object appears entirely nebular,…

天体物理学 · 物理学 2009-11-13 Richard A. Shaw , Armin Rest , Guillermo Damke , R. Chris Smith , Warren A. Reid , Quentin A. Parker

In this paper we explore the dynamics of ionization bounded planetary nebulae after the termination of the fast stellar wind. When the stellar wind becomes negligible, the hot, shocked bubble depressurizes and the thermal pressure of the…

天体物理学 · 物理学 2009-11-11 G. Garcia-Segura , J. A. Lopez , W. Steffen , J. Meaburn , A. Manchado

The curious Galactic features near G357.2$-$0.2 were observed with the MeerKAT radio interferometer array in the UHF and L bands (0.56--1.68 GHz). There are two possibly related features: a newly identified faint heart-shaped partial shell…

高能天体物理现象 · 物理学 2022-08-03 W. D. Cotton , F. Camilo , W. Becker , J. J. Condon , J. Forbrich , I. Heywood , B. Hugo , S. Legodi , T. Mauch , P. Predehl , P. Slane , M. A. Thompson

Bow-shock pulsar wind nebulae (PWNe) show a variety of morphological shapes. We attribute this diversity to the geometrical factors: relative orientations of the pulsar rotation axis, proper velocity, and the line of sight (magnetic…

高能天体物理现象 · 物理学 2019-01-30 Maxim V. Barkov , Maxim Lyutikov , Dmitry Khangulyan

We present the results of differential proper-motion analyses of the Egg Nebula (RAFGL 2688, V1610 Cyg) based on the archived two-epoch optical data taken with the Hubble Space Telescope. First, we determined that the polarization…

太阳与恒星天体物理 · 物理学 2015-06-16 Toshiya Ueta , Rachael L. Tomasino , Brian A. Ferguson

We present a morphological study of nebulae around Wolf-Rayet (WR) stars using archival narrow-band optical and Wide-field Infrared Survey Explorer (WISE) infrared images. The comparison among WISE images in different bands and optical…

太阳与恒星天体物理 · 物理学 2015-06-17 J. A. Toalá , M. A. Guerrero , G. Ramos-Larios , V. Guzmán

We discuss the formation of globules in planetary nebulae, typified by those observed in the Helix Nebula. We show that the properties of the globules, their number, mass, separation, and overall geometry strongly support a scenario in…

天体物理学 · 物理学 2009-11-11 P. J. Huggins , A. Frank