中文
相关论文

相关论文: A carbon-rich hot bubble in the planetary nebula N…

200 篇论文

We report the discovery of X-ray emission from NGC 7027, a prototypical object for the study of the formation and evolution of planetary nebulae (PNs). Observations with the Advanced CCD Imaging Spectrometer (ACIS) aboard the Chandra X-ray…

天体物理学 · 物理学 2009-11-06 Joel H. Kastner , Saeqa D. Vrtilek , Noam Soker

XMM-Newton EPIC observations of the planetary nebula (PN) NGC 7009, the Saturn Nebula, have detected extended X-ray emission in its central cavity. The diffuse X-ray emission must originate in the shocked fast stellar wind. The spectra show…

天体物理学 · 物理学 2009-11-07 Martin A. Guerrero , Robert A. Gruendl , You-Hua Chu

We present deep XMM-Newton EPIC observations of the Wolf-Rayet (WR) bubble NGC6888 around the star WR136. The complete X-ray mapping of the nebula confirms the distribution of the hot gas in three maxima spatially associated with the caps…

太阳与恒星天体物理 · 物理学 2016-01-20 J. A. Toalá , M. A. Guerrero , Y. -H. Chu , S. J. Arthur , D. Tafoya , R. A. Gruendl

We report the serendipitous detection of the planetary nebula NGC 5315 by the Chandra X-ray Observatory. The Chandra imaging spectroscopy results indicate that the X-rays from this PN, which harbors a Wolf-Rayet (WR) central star, emanate…

天体物理学 · 物理学 2012-08-27 Joel Kastner , Rodolfo Montez, , Bruce Balick , Orsola De Marco

The Wolf-Rayet (WR) nebula NGC3199 has been suggested to be a bow shock around its central star WR18, presumably a runaway star, because optical images of the nebula show a dominating arc of emission south-west of the star. We present the…

太阳与恒星天体物理 · 物理学 2017-09-13 J. A. Toalá , A. P. Marston , M. A. Guerrero , Y. -H. Chu , R. A. Gruendl

The planetary nebula (PN) NGC 5189 around a Wolf-Rayet [WO] central star demonstrates one of the most remarkable complex morphologies among PNe with many multi-scale structures, showing evidence of multiple outbursts from an AGB progenitor.…

太阳与恒星天体物理 · 物理学 2018-01-11 Ashkbiz Danehkar , Margarita Karovska , W. Peter Maksym , Rodolfo Montez

We report the serendipitous detection by the XMM-Newton X-ray Observatory of an X-ray source at the position of the Type I (He- and N-rich) bipolar planetary nebula Hb 5. The Hb 5 X-ray source appears marginally resolved. While the small…

太阳与恒星天体物理 · 物理学 2011-02-11 Rodolfo Montez , Joel H. Kastner , Bruce Balick , Adam Frank

We present analysis of a second observation of the young planetary nebula (PN) NGC 7027 by the Chandra X-ray Observatory. This latest 59.2 ks exposure with ACIS-S was acquired approximately 14 years after the initial 18.2 ks ACIS-S…

太阳与恒星天体物理 · 物理学 2018-07-18 Rodolfo Montez , Joel H. Kastner

We present new XMM-Newton observation of the Ultra Luminous Infrared Galaxy (ULIRG) NGC 6240. We analyze the reflecting grating spectrometer (RGS) data, and data from the other instruments, and find a starburst dominated 0.5-3 keV spectrum…

天体物理学 · 物理学 2009-11-11 Hagai Netzer , Doron Lemze , Shai Kaspi , I. M. George , T. J. Turner , D. Lutz , T. Boller , Doron Chelouche

We present a set of optical and infrared images combined with long-slit, medium and high dispersion spectra of the southern planetary nebula (PN) NGC 5189. The complex morphology of this PN is puzzling and has not been studied in detail so…

太阳与恒星天体物理 · 物理学 2012-03-07 L. Sabin , R. Vázquez , J. A. López , Ma. T. García-Díaz , G. Ramos-Larios

We revisit Chandra observations of the planetary nebulae NGC 7027 and BD +30 3639 in order to address the question of abundance anomalies in the X-ray emitting gas. Enhanced abundances relative to solar of magnesium (Mg) for NGC 7027 and…

天体物理学 · 物理学 2009-11-07 Holly L. Maness , Saeqa D. Vrtilek , Noam Soker , Joel H. Kastner

We present the first high-resolution X-ray spectrum of the Seyfert 1.5 galaxy NGC 4151. Observations with the Chandra High Energy Transmission Grating Spectrometer reveal a spectrum dominated by narrow emission lines from a spatially…

天体物理学 · 物理学 2009-10-31 P. M. Ogle , H. L. Marshall , J. C. Lee , C. R. Canizares

We report the radio continuum detection of well known Galactic Planetary Nebula (PN) NGC 5189, observed at 943 MHz during the Australian Square Kilometre Array Pathfinder (ASKAP) Evolutionary Map of the Universe (EMU) survey. Two detections…

星系天体物理 · 物理学 2025-08-06 A. D. Asher , Z. J. Smeaton , M. D. Filipović , A. M. Hopkins , J. Th. van Loon , T. J. Galvin , L. A. Barnes

XMM-Newton observations of the starburst galaxy NGC 1511 reveal the presence of a previously unknown extended hot gaseous phase of its ISM, which partly extends out of the disk plane. The emission distribution is asymmetric, being brightest…

天体物理学 · 物理学 2008-11-26 M. Dahlem , M. Ehle , F. Jansen , T. M. Heckman , K. A. Weaver , D. K. Strickland

One key feature of the interacting stellar winds model of the formation of planetary nebulae (PNe) is the presence of shock-heated stellar wind confined in the central cavities of PNe. This so-called hot bubble should be detectable in…

高能天体物理现象 · 物理学 2015-05-28 Nieves Ruiz , Martin A. Guerrero , You-Hua Chu , Robert A. Gruendl

We discuss our most recent findings on the diffuse X-ray emission from Wolf-Rayet (WR) nebulae. The best-quality X-ray observations of these objects are those performed by XMM-Newton and Chandra towards S308, NGC2359, and NGC6888. Even…

高能天体物理现象 · 物理学 2015-11-04 J. A. Toalá , M. A. Guerrero , Y. -H. Chu , S. J. Arthur , R. A. Gruendl

We present the results from coordinated X-ray observations of the ultraluminous X-ray source NGC 5204 X-1 performed by NuSTAR and XMM-Newton in early 2013. These observations provide the first detection of NGC 5204 X-1 above 10 keV,…

Chandra X-ray Observatory (CXO) images have revealed that the X-ray emitting regions of the molecule-rich young planetary nebulae (PNs) BD+30 3639 (BD+30) and NGC 7027 are much more asymmetric than their optical nebulosities. To evaluate…

天体物理学 · 物理学 2009-11-07 Joel H. Kastner , Jingqiang Li , Saeqa D. Vrtilek , Ian Gatley , K. M. Merrill , Noam Soker

We report on X-ray emission from the Seyfert 2 galaxy NGC4388 observed with the Chandra X-ray Observatory. A hard X-ray peak is found at the position of the active nucleus suggested by optical and radio observations. Extended soft X-ray…

天体物理学 · 物理学 2009-09-17 K. Iwasawa , A. S. Wilson , A. C. Fabian , A. J. Young

We present the results of the first X-ray gratings spectroscopy observations of a planetary nebula (PN), the X-ray-bright, young BD+30 3639. We observed BD+30 3639 for a total of 300 ks with the Chandra X-ray Observatory's Low Energy…

天体物理学 · 物理学 2008-12-18 Young Sam Yu , Raanan Nordon , Joel H. Kastner , John Houck , Ehud Behar , Noam Soker
‹ 上一页 1 2 3 10 下一页 ›