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Related papers: Multiple and Precessing Collimated Outflows in the…

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We present new results on the nature of the Herbig-Haro-like object 73 (HHL73, also known as [G84b] 11) based on narrow-band CCD H_alpha and [SII] images of the HHL73 field, and Integral Field Spectroscopy and radio continuum observations…

Astrophysics · Physics 2009-11-13 R. Lopez , S. F. Sanchez , B. Garcia-Lorenzo , R. Estalella , A. Riera , G. Busquet

This study aims to probe the thermodynamic properties of the hot intragroup medium (IGM) plasma in the core regions of the NGC 4636 galaxy group by detailed measurements of several emission lines and their relative intensities. We analyzed…

High Energy Astrophysical Phenomena · Physics 2016-07-27 Jussi Ahoranta , Alexis Finoguenov , Ciro Pinto , Jeremy Sanders , Jelle Kaastra , Jelle de Plaa , Andrew Fabian

The structure of the dusty circumstellar envelopes (CSEs) of proto-planetary nebulae (PPNs) reveals the mass-loss history of these sources and how such histories may differ for elliptical (SOLE) and bipolar (DUPLEX) PPNs. To study the PPN…

Astrophysics · Physics 2008-11-26 Toshiya Ueta , Koji Murakawa , Margaret Meixner

We present the results of a detailed investigation into the physical conditions in interstellar material interacting with the supernova remnant IC 443. Our analysis is based on a comprehensive examination of high-resolution far-ultraviolet…

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…

Solar and Stellar Astrophysics · Physics 2022-03-14 G. Ramos-Larios , J. A. Toalá , J. B. Rodríguez-González , M. A. Guerrero , V. M. A. Gómez-González

Shell-type supernova remnants (SNRs) accelerate particles at the shock front between the expanding remnant and the swept-up interstellar medium. If these particles include protons and nuclei, very-high-energy gamma-ray emission may result…

Astrophysics · Physics 2007-09-28 VERITAS Collaboration , T. B. Humensky

We find in a detailed morphological study (at 15 pc resolution) that the extended massive star formation process, shows: (i) extended triple asymmetrical spiral arms structure (r = 5 kpc); and (ii) the spiral arms emanate from three…

Astrophysics · Physics 2009-10-31 S. Lipari , R. Diaz , Y. Taniguchi , R. Terlevich , H. Dottori , G. Carranza

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…

Studies of brown dwarf (BD) outflows provide information pertinent to questions on BD formation, as well as allowing outflow mechanisms to be investigated at the lowest masses. Here new observations of the bipolar outflow from the 24…

Solar and Stellar Astrophysics · Physics 2015-06-11 Emma Whelan , Tom Ray , Fernando Comeron , Francesca Bacciotti , Patrick Kavanagh

The multiple protostellar system L1551 IRS5 exhibits a large-scale bipolar molecular outflow. We have studied this outflow within ~4000 AU of its driving source(s) with the SubMillimeter Array. Our CO(2-1) image at ~4" (~560 AU) resolution…

Solar and Stellar Astrophysics · Physics 2011-02-11 Po-Feng Wu , Shigehisa Takakuwa , Jeremy Lim

We present Submillimeter Array (SMA) mapping of $^{12}$CO $J=2\rightarrow 1$, $^{13}$CO $J=2\rightarrow 1$, and CN $N=2\rightarrow 1$ emission from the Ring-like planetary nebula (PN) NGC 3132, one of the subjects of JWST Early Release…

Solar and Stellar Astrophysics · Physics 2024-02-21 Joel H. Kastner , David Wilner , Paula Moraga Baez , Jesse Bublitz , Orsola De Marco , Raghvendra Sahai , Al Wootten

The planetary nebula (PN) Abell 48 (PN G029.0+00.4) is around a rare Wolf-Rayet [WN5] star whose stellar history is as yet unknown. Using the integral field observations of the H$\alpha$ $\lambda$6563 and [N II] $\lambda$6584 line…

Solar and Stellar Astrophysics · Physics 2022-02-16 A. Danehkar

HST NICMOS narrowband images of the shocked molecular hydrogen emission in OMC-1 are analyzed to reveal new information on the BN/KL outflow. The outstanding morphological feature of this region is the array of molecular hydrogen…

This work presents three dimensional, magneto-hydrodynamical simulations of the formation and early evolution of a subgroup of planetary nebulae that exhibit a variety of point-symmetric structures. For bipolar nebulae, the formation of…

Astrophysics · Physics 2016-08-15 G. García-Segura , J. A. López

Interaction between a central outflow and a surrounding wind is common in astrophysical sources powered by accretion. Understanding how the interaction might help to collimate the inner central outflow is of interest for assessing…

High Energy Astrophysical Phenomena · Physics 2015-06-19 R. Yurchak , A. Ravasio , A. Pelka , S. Pikuz , E. Falize , T. Vinci , M. Koenig , B. Loupias , A. Benuzzi-Mounaix , M. Fatenejad , P. Tzeferacos , D. Q. Lamb , E. G. Blackman

The young, compact, very high surface brightness but low excitation planetary nebula (PN) BD+303639 is one of the very few PNe that have been reported to exhibit the 21cm HI emission line. As part of a long-term programme to search for…

Solar and Stellar Astrophysics · Physics 2023-08-02 Xu-Jia Ouyang , Yong Zhang , Albert Zijlstra , Chuan-Peng Zhang , Jun-ichi Nakashima , Quentin A Parker

New radio continuum (8 GHz and 1.4 GHz) and HI 21 cm line observations of the Seyfert 2 galaxy IC 5063 (PKS 2048-572) were obtained with the Australia Telescope Compact Array (ATCA). The 8 GHz image reveals a linear triple structure (~4'',…

Astrophysics · Physics 2009-10-30 R. Morganti , T. Oosterloo , Z. Tsvetanov

We report high angular-resolution (~1") CO J=3--2 interferometric mapping, using the Submillimeter Array (SMA), of IRAS22036+5306 (I22036), a bipolar pre-planetary nebula (PPN) with knotty jets discovered in our HST SNAPshot survey of young…

Astrophysics · Physics 2008-11-26 R. Sahai , K. Young , N. A. Patel , C. S'anchez Contreras , M. Morris

We present line and continuum observations made with the Submillimeter Array (SMA) of the young stellar object Barnard 5 - IRS1 located in the Perseus molecular cloud. Our $^{12}$CO(2-1) line observations resolve the high-velocity bipolar…

Solar and Stellar Astrophysics · Physics 2015-06-19 Luis A. Zapata , Hector G. Arce , Erin Brassfield , Aina Palau , Nimesh Patel , Jaime E. Pineda