Výsledky vyhledávání - "Jets And Outflows, [Ism]"

Chemistry and physical properties of the born-again planetary nebula HuBi 1

Autor: B Montoro-Molina, M A Guerrero, B Pérez-Díaz, J A Toalá, S Cazzoli, M M Miller Bertolami, C Morisset

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
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The central star of the planetary nebula (PN) HuBi 1 has been recently proposed to have experienced a very late thermal pulse (VLTP), but the dilution of the emission of the recent ejecta by that of the surrounding H-rich old outer shell has so far h

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d5ed3a4ec0749dc50420d7c16d468aa
https://doi.org/10.1093/mnras/stac336

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Akademický článek

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CHANG-ES XXIX: the sub-kpc nuclear bubble of NGC 4438

Autor: Jiang-Tao Li, Q Daniel Wang, Theresa Wiegert, Joel N Bregman, Rainer Beck, Ancor Damas-Segovia, Judith A Irwin, Li Ji, Yelena Stein, Wei Sun, Yang Yang

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
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Active galactic nucleus (AGN) bubbles could play an important role in accelerating high-energy cosmic rays (CRs) and galactic feedback. Only in nearby galaxies could we have high enough angular resolution in multiwavelengths to study the sub-kpc envi

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a34a26e536f12fd4708da8099bfd7762
http://hdl.handle.net/10261/282802

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The structure of jets launched from post-AGB binary systems

Autor: Mark Wardle, Olivier Verhamme, Anne Verhamme, Jacques Kluska, Devika Kamath, Hans Van Winckel, Orsola De Marco

We focus on post-asymptotic giant branch (post-AGB) binaries and study the interaction between the different components of these complex systems. These components comprise the post-AGB primary, a main sequence secondary, a circumbinary disk, as well

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c6d0a3ce080f60b81120551379132b34
http://arxiv.org/abs/2208.08752

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Rapid compact jet quenching in the Galactic black hole candidate X-ray binary MAXI J1535−571

Publikováno v: Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 498 (4), pp.5772-5785. ⟨10.1093/mnras/staa2650⟩
Monthly Notices of the Royal Astronomical Society, 498(4), 5772-5785. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 498 (4), pp.5772-5785. ⟨10.1093/mnras/staa2650⟩

We present results from six epochs of quasi-simultaneous radio, (sub-)millimetre, infrared, optical, and X-ray observations of the black hole X-ray binary MAXI~J1535$-$571. These observations show that as the source transitioned through the hard-inte

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::258218cf886296185e034c1684f4a8b3
https://doi.org/10.1093/mnras/staa2650

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Progenitor, precursor, and evolution of the dusty remnant of the stellar merger M31-LRN-2015

Autor: Peter Nugent, J. E. Jencson, Mansi M. Kasliwal, Christopher S. Kochanek, Karambelkar, Frank J. Masci, Joel Johansson, Scott M. Adams, S. Kozlowski, Nadejda Blagorodnova, H Campbell, Umaa Rebbapragada, R. R. Laher, Subo Dong, Simon Hodgkin

Publikováno v: Monthly Notices of the Royal Astronomical Society, vol 496, iss 4

M31-2015-LRN is a likely stellar merger discovered in the Andromeda Galaxy in 2015. We present new optical to mid-infrared photometry and optical spectroscopy for this event. Archival data shows that the source started to brighten $\sim$2 years befor

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::07ab51def941e79084a0182a52945366
https://doi.org/10.1093/mnras/staa1872

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Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)

Autor: Wouter Vlemmings, Jaeheon Kim, Jorge Cantó, N. Añez-López, G. Surcis, Soon-Wook Kim, Salvador Curiel, Adriana R Rodríguez-Kamenetzky, José-Luis Gómez, Ciriaco Goddi, Luis F. Rodríguez, Carlos Carrasco-González, José M. Torrelles, H. J. van Langevelde

Publikováno v: CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Monthly Notices of the Royal Astronomical Society, 496(3), 3128-3141
Digital.CSIC. Repositorio Institucional del CSIC
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Monthly Notices of the Royal Astronomical Society, 496, 3128-3141
Monthly Notices of the Royal Astronomical Society, 496, 3, pp. 3128-3141

The massive star-forming region W75N (B) is thought to host a cluster of massive protostars (VLA 1, VLA 2, and VLA 3) undergoing different evolutionary stages. In this work, we present radio continuum data with the highest sensitivity and angular res

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b938485f2764af757015f5931937482a
https://doi.org/10.1093/mnras/staa1742

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Rapid particle acceleration due to recollimation shocks and turbulent magnetic fields in injected jets with helical magnetic fields

Autor: Martin Pohl, José L. Gómez, Jacek Niemiec, Kouichi Hirotani, Nicholas R. MacDonald, Ioana Duţan, Oleh Kobzar, Yosuke Mizuno, A. Meli, Ken-Ichi Nishikawa

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
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This article has been accepted for publication in MNRAS © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
One of the key questions in the study of relativistic jets is how magnetic reconnectio

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8f9ddcc9cc723d96e5c1fed35393944
https://doi.org/10.1093/mnras/staa421

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Collision of protostellar jets in the star-forming region IC 1396N

Autor: López, Rosario, Estalella, Robert, Beltrán, María Teresa, Massi, Fabrizio, Acosta, Jose A., Girart, Josep Miquel

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
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[Context] The bright-rimmed cloud IC 1396N is believed to host one of the few known cases where two bipolar CO outflows driven by young stellar objects collide. The CO outflows are traced by chains of knots of H2 emission, with enhanced emission at t

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::3a2cae2ebbdde1d34a2194ab6c31a746
http://hdl.handle.net/10261/276322

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Cool outflows in MaNGA: a systematic study and comparison to the warm phase

Autor: Charlotte R Avery, Stijn Wuyts, Natascha M Förster Schreiber, Carolin Villforth, Caroline Bertemes, Stephen L Hamer, Raman Sharma, Jun Toshikawa, Junkai Zhang

Publikováno v: Avery, C R, Wuyts, S, Förster schreiber, N M, Villforth, C, Bertemes, C, Hamer, S L, Sharma, R, Toshikawa, J & Zhang, J 2022, ' Cool outflows in MaNGA : a systematic study and comparison to the warm phase ', Monthly Notices of the Royal Astronomical Society, vol. 511, no. 3, pp. 4223-4237 . https://doi.org/10.1093/mnras/stac190

This paper investigates the neutral gas phase of galactic winds via the Na I D$\lambda\lambda 5890,5895${\AA} feature within $z \sim 0.04$ MaNGA galaxies, and directly compares their incidence and strength to the ionized winds detected within the sam

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5cb1e0a6ddbca8ee70508f3255ffa034
http://arxiv.org/abs/2201.08079

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