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Related papers: H$_2$ in low-ionization structures of planetary ne…

200 papers

We report results from a Hubble Space Telescope (HST) and Near-Infrared Camera and Multiobject Spectrometer (NICMOS) program to study the distribution of hot neutral (molecular hydrogen) and ionized circumstellar material in the young…

We present narrow-band optical images, VLA-A 3.6 cm continuum and H92alpha emission line data and high resolution long-slit [N II] spectra of Hu 2-1. The formation of Hu 2-1 appears dominated by anisotropic mass ejection during the late AGB…

21cm spectral-line and continuum observations of ten compact planetary nebulae have been made with the Very Large Array. Circumnebular atomic hydrogen is identified in the planetary nebulae SwSt1, M3-35, and possibly in Hu2-1. The…

Astrophysics · Physics 2015-06-24 G. T. Gussie , A. R. Taylor

NGC 6369 is a double-shell planetary nebula (PN) consisting of a bright annular inner shell with faint bipolar extensions and a filamentary envelope. We have used ground- and space-based narrow-band optical and near-IR images, broad-band…

Solar and Stellar Astrophysics · Physics 2015-06-03 Gerardo Ramos-Larios , Martin A. Guerrero , Roberto Vazquez , J. P. Phillips

We present results from integral field optical spectroscopy with the Potsdam Multi-Aperture Spectrograph of the Herbig-Haro (HH) object HH 204, with a spatial sampling of 1 x 1 arcsec^2. We have obtained maps of different emission lines,…

Astrophysics of Galaxies · Physics 2015-06-03 M. Núñez-Díaz , A. Mesa-Delgado , C. Esteban , L. López-Martín , J. García-Rojas , V. Luridiana

To investigate the presence of small scale structure in the spatial distribution of H2 molecules we have undertaken repeated FUSE UV observations of the runaway O9.5V star, HD34078. In this paper we present five spectra obtained between…

We report the detection during the Chandra Orion Ultradeep Project (COUP) of two soft, constant, and faint X-ray sources associated with the Herbig-Haro object HH210. HH210 is located at the tip of the NNE finger of the emission line system…

Around 50 PNe are presently known to possess "small-scale" low-ionization structures (LISs). We consider here jets, jet-like, symmetrical and non-symmetrical LISs and present a detailed comparison of the existing model predictions with the…

Astrophysics · Physics 2009-10-31 Denise R. Goncalves , Romano L. M. Corradi , Antonio Mampaso

SBS0335-052E, one of the most metal-poor (Z ~ 3-4% Z$_{\odot}$) HeII-emitter starbursts known in the nearby universe, is studied using optical VLT/MUSE spectroscopic and Chandra X-ray observations. We spatially resolved the spectral map of…

Astrophysics of Galaxies · Physics 2018-08-01 C. Kehrig , J. M. Vilchez , M. A. Guerrero , J. Iglesias-Paramo , L. K. Hunt , S. Duarte Puertas , G. Ramos-Larios

ABRIDGED: 2D spectroscopic MUSE data for the whole extent of NGC3132 have been reduced and analised. The dust extinction, electron densities and temperatures of the ionised gas and abundances were determined. The nebula presents a complex…

Solar and Stellar Astrophysics · Physics 2020-02-05 Ana Monreal-Ibero , Jeremy R. Walsh

We present a new analysis of the physical conditions in three Herbig-Haro complexes (HH 54, HH 212, and the L 1157 protostellar jet) using archival data from the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. As described in…

Solar and Stellar Astrophysics · Physics 2015-05-30 Michihiro Takami , Jennifer L. Karr , Brunella Nisini , Thomas P. Ray

We investigate the ionization structure of the nebular gas in M83 using the line diagnostic diagram, [O III](5007 \degA)/H{\beta} vs. [S II](6716 \deg A+6731 \deg A)/H{\alpha} with the newly available narrowband images from the Wide Field…

Stellar mergers produce explosive outflows that serve as transient sources of IR line luminosity and inject mechanical energy early into the natal molecular cloud. We present the first velocity-resolved maps of the [O I] 63 and 145 um…

Astrophysics of Galaxies · Physics 2026-05-27 J. R. Goicoechea , R. Güsten , B. Godard , H. Wiesemeyer , R. Higgins , A. Gusdorf , M. G. Santa-Maria , M. Zannese , K. M. Menten

In this contribution, I will briefly review the development of the theory of photoionized gaseous nebulae, highlighting some of the key events. I will then present some recent developments of deep spectroscopy of planetary nebulae (PNe) and…

Astrophysics of Galaxies · Physics 2010-02-23 Xiaowei Liu

We present [N II] and H-alpha images and high resolution long-slit spectra of the planetary nebula IC 4846, which reveal, for the first time, its complex structure and the existence of collimated outflows. The object consists of a…

Astrophysics · Physics 2009-10-31 Luis F. Miranda , Martin A. Guerrero , Jose M. Torrelles

This work presents integrated flux and velocity channel maps of the planetary nebula Abell 30 (A30) inner knot system. The observations were taken with the INTEGRAL spectrograph at the William Herschel Telescope (WHT). Our IFU data cube…

Astrophysics of Galaxies · Physics 2026-02-06 Kam Ling Chan , Andreas Ritter , Quentin Andrew Parker , Katrina Exter

We report the detection of a highly collimated linear emission-line structure in the spiral galaxy NGC\,232 through the use of integral field spectroscopy data from the All-weather MUse Supernova Integral field Nearby Galaxies (AMUSING)…

We present HST STIS observations of two extreme NLS1s, IRAS 13224-3809 and 1H 0707-495. The spectra are characterized by very blue continua, broad, strongly blueshifted high-ionization lines (including \ion{C}{4} and \ion{N}{5}), and…

Astrophysics · Physics 2009-11-10 Karen M. Leighly , John R. Moore

We have mapped the Helix (NGC 7293) planetary nebula (PN) with the IRAC instrument on the Spitzer Space Telescope. The Helix is one of the closest bright PN, and therefore provides an opportunity to resolve the small-scale structure in the…

Astrophysics · Physics 2008-11-26 Joseph L. Hora , William B. Latter , Howard A. Smith , Massimo Marengo

We report the first detection of optical emission from the shell-type Galactic supernova remnant (SNR) G108.2$-$0.6. We obtained H$\alpha$ images and long-slit spectra using the 1.5-m RTT150 telescope to examine the morphological and…

High Energy Physics - Phenomenology · Physics 2023-12-21 Gunay Payli , Hicran Bakis , Ebru Aktekin , Hidetoshi Sano , Aytap Sezer