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Direct imagery and long-slit, spatially resolved echellograms of the high excitation planetary nebula NGC 1501 allowed us to study in detail the expansion velocity field, the physical conditions (electron temperature, electron density,…

天体物理学 · 物理学 2007-05-23 Franco Sabbadin , Stefano Benetti , Enrico Cappellaro , Massimo Turatto

We have conducted a detailed multi-wavelength study of the peculiar nebula Abell 48 and its central star. We classify the nucleus as a helium-rich, hydrogen-deficient star of type [WN4-5]. The evidence for either a massive WN or a low-mass…

太阳与恒星天体物理 · 物理学 2015-12-09 David J. Frew , Ivan S. Bojicic , Q. A. Parker , M. Stupar , S. Wachter , K. DePew , A. Danehkar , M. T. Fitzgerald , D. Douchin

We present a detailed analysis of deep VLT/X-Shooter observations of the planetary nebula Tc 1. We calculate gas temperature, density, extinction, and abundances for several species from the empirical analysis of the total line fluxes. In…

We have carried out optical observations of the north-eastern part of the supernova remnant IC 443 using the CFHT imaging spectrograph SITELLE. The observations consist of three multispectral cubes covering an 11$^{\prime}$…

星系天体物理 · 物理学 2019-09-04 Alexandre Alarie , Laurent Drissen

We analyze the chemical composition of the central star of the planetary nebula NGC 6543 based upon a detailed NLTE model of its stellar wind. The logarithmic abundances by number are H=12.00, He=11.00, C=9.03, N=8.36, O=9.02, Si=8.19,…

天体物理学 · 物理学 2009-11-13 L. N. Georgiev , M. Peimbert , D. J. Hillier , M. G. Richer , A. Arrieta , A. Peimbert

The iconic planetary nebula (PN) NGC 7027 is bright, nearby (D ~ 1 kpc), highly ionized, intricately structured, and well observed. This nebula is hence an ideal case study for understanding PN shaping and evolution processes. Accordingly,…

星系天体物理 · 物理学 2023-01-04 Paula Moraga Baez , Joel H. Kastner , Bruce Balick , Rodolfo Montez , Jesse Bublitz

The study presents a detailed spectroscopic analysis of the planetary nebulae (PNe) NGC~2392 and NGC~4361 using optical spectra obtained from the 2-m Himalayan Chandra Telescope (HCT) and mid-infrared spectra from archival \textit{Spitzer}…

太阳与恒星天体物理 · 物理学 2025-10-17 Atul Kumar Singh , Saurabh Sharma , Rahul Kumar Anand , Arpan Ghosh , Tarak Chand , Shantanu Rastogi

We present Herschel PACS and SPIRE images of the dust shells around the planetary nebulae NGC 650, NGC 6853, and NGC 6720, as well as images showing the dust temperature in their shells. The latter shows a rich structure, which indicates…

太阳与恒星天体物理 · 物理学 2015-05-30 G. C. Van de Steene , K. M. Exter , P. A. M. van Hoof , T. L. Lim , M. J. Barlow , M. Matsuura , T. Ueta , the MESS Consortium

We investigate the structure of the planetary nebula (PN) NGC 2371 using [OIII]-5007 imaging taken with the Jacobus Kapteyn 1.0 m telescope, and [NII]-6584, [OIII]-5007 and Ha results acquired with the Hubble Space Telescope (HST). These…

星系天体物理 · 物理学 2015-06-05 G. Ramos-Larios , J. P. Phillips

We present medium-dispersion spectra and narrowband images of six northern compact planetary nebulae (PNe): BoBn 1, DdDm 1, IC 5117, M 1-5, M 1-71, and NGC 6833. From broad-slit spectra, total absolute fluxes and equivalent widths were…

天体物理学 · 物理学 2009-11-11 S. A. Wright , R. L. M. Corradi , M. Perinotto

The central regions of galaxies harbouring active galactic nuclei (AGNs) can be quite complex, especially at high activity, presenting, besides variability, a variety of phenomena related, e.g. to ionization/excitation mechanisms. A…

The spectra of the planetary nebula NGC2392 is reanalysed using spectral measurements made in the mid-infrared with the Spitzer Space Telescope. The aim is to determine the chemical composition of this object. We also make use of IUE and…

天体物理学 · 物理学 2009-11-13 S. R. Pottasch , J. Bernard-Salas , T. L. Roellig

In this study, we present the results of photoionization modeling for 124 planetary nebulae (PNe) in the Galactic bulge. Utilizing the {\scshape cloudy} code, we derived the effective temperatures (T$_{eff}$) of the central stars, with a…

星系天体物理 · 物理学 2025-10-21 N. Aksaker , A. Demirci , N. Erzincan , A. Akyuz

This paper presents new near-infrared observations of the planetary nebula NGC 2346. The data include a broad K-band image, an image in the H2 vibrationally excited 1-0S(1) line and K band slit spectra at three positions in the nebula. In…

天体物理学 · 物理学 2007-05-23 B. Vicini , A. Natta , A. Marconi , L. Testi , D. Hollenbach , B. T. Draine

We conducted research on the classification and physical properties of 10 objects from the HASH (Hong Kong/Australian Astronomical Observatory/Strasbourg Observatory H-alpha Planetary Nebula (PN)) database with small angular sizes (<…

太阳与恒星天体物理 · 物理学 2023-09-28 Utkan Temiz , Nazım Aksaker , Aysun Akyuz

This work aims to search for the observational footprints of the interactions between the interstellar medium (ISM) and stellar winds in the Wolf-Rayet (WR) nebula NGC6888 in order to understand its ionization structure, chemical…

Knots are commonly found in nearby planetary nebulae (PNe) and star forming regions. Within PNe, knots are often found to be associated with the brightest parts of the nebulae and understanding the physics involved in knots may reveal the…

天体物理学 · 物理学 2009-11-13 M. Matsuura , A. K. Speck , M. D. Smith , A. A. Zijlstra , S. Viti , K. T. E. Lowe , M. Redman , C. J. Wareing , E. Lagadec

We present high-resolution images of the strongly bipolar planetary nebula NGC 6537, obtained with Hubble Space Telescope and with the infrared adaptive optics system on the Very Large Telescope. The central star is detected for the first…

天体物理学 · 物理学 2009-11-13 M. Matsuura , A. A. Zijlstra , M. D. Gray , F. J. Molster , L. B. F. M. Waters

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 compile published spectroscopic data and [O III] magnitudes of almost 500 extragalactic planetary nebulae (PNe) in 13 galaxies of various masses and morphological types. This is the first paper of a series that aims to analyze the PN…