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Related papers: Nebular vs. Stellar Wind Abundances in NGC 6543

200 papers

We present comprehensive X-ray point source catalogs of NGC~55, NGC~2403, and NGC~4214 as part of the Chandra Local Volume Survey. The combined archival observations have effective exposure times of 56.5 ks, 190 ks, and 79 ks for NGC~55,…

High Energy Astrophysical Phenomena · Physics 2015-09-16 B. Binder , B. F. Williams , M. Eracleous , P. P. Plucinsky , T. J. Gaetz , S. F. Anderson , E. D. Skillman , J. J. Dalcanton , A. K. H. Kong , D. R. Weisz

We report the detection of well resolved, extended X-ray emission from the young planetary nebula BD+303639 using the Advanced CCD Imaging Spectrometer (ACIS) aboard the Chandra X-ray Observatory. The X-ray emission from BD+303639 appears…

Astrophysics · Physics 2009-10-31 Joel H. Kastner , Noam Soker , Saeqa Vrtilek , Ruth Dgani

The cluster NGC 3603 hosts some of the most massive stars in the Galaxy. With a modest 50 ks exposure with the Chandra High Energy Grating Spectrometer, we have resolved emission lines in spectra of several of the brightest cluster members…

Solar and Stellar Astrophysics · Physics 2019-01-09 David P. Huenemoerder , Norbert S. Schulz , Joy S. Nichols

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…

High Energy Astrophysical Phenomena · Physics 2015-05-28 Nieves Ruiz , Martin A. Guerrero , You-Hua Chu , Robert A. Gruendl

We present preliminary results from a systematic spectral study of pulsars and their wind nebulae using the Chandra X-Ray Observatory. The superb spatial resolution of Chandra allows us to differentiate the compact object's spectrum from…

Astrophysics · Physics 2007-05-23 E. V. Gotthelf , C. M. Olbert

We present CHANDRA X-ray data of the nearby Magellanic Irregular dwarf starburst galaxy NGC4449. Contributions to the X-ray emission come from discrete point sources and extended diffuse emission. The extended emission has a complex…

Astrophysics · Physics 2009-11-07 Lesley K. Summers , Ian R. Stevens , David K. Strickland , Timothy M. Heckman

We present a brief review of Chandra X-ray Observatory observations of neutron stars. The outstanding spatial and spectral resolution of this great observatory have allowed for observations of unprecedented clarity and accuracy. Many of…

Astrophysics · Physics 2008-11-26 M. C. Weisskopf , M. Karovska , G. G. Pavlov , V. E. Zavlin , T. Clarke

We report the discovery, by the Chandra X-ray Observatory, of X-ray emission from the bipolar planetary nebula Menzel 3. In Chandra CCD imaging, Mz 3 displays hot (3-6x10^6 K) gas within its twin, coaxial bubbles of optical nebulosity, as…

We present Chandra and XMM-Newton X-ray data of NGC5253, a local starbursting dwarf elliptical galaxy, in the early stages of a starburst episode. Contributions to the X-ray emission come from discrete point sources and extended diffuse…

Astrophysics · Physics 2009-11-10 Lesley K. Summers , Ian R. Stevens , David K. Strickland , Timothy M. Heckman

A Chandra observation of the isolated hard X-ray source XMMU J061804.3+222732, located in the region of apparent interaction of the supernova remnant IC 443 with a molecular cloud, resolved the complex structure of the source in a few…

Astrophysics · Physics 2009-11-10 A. M. Bykov , F. Bocchino , G. G. Pavlov

We have obtained X-ray observations of the bipolar planetary nebulae (PNe) NGC 2346 and NGC 7026 with XMM-Newton. These observations detected diffuse X-ray emission from NGC 7026 but not from NGC 2346. The X-ray emission from NGC 7026…

Astrophysics · Physics 2007-05-23 Robert A. Gruendl , Martin A. Guerrero , You-Hua Chu , Rosa M. Williams

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…

Solar and Stellar Astrophysics · Physics 2011-02-11 Rodolfo Montez , Joel H. Kastner , Bruce Balick , Adam Frank

We report the detection of a point source CXO J172337.5-373442 in a Chandra field with a high significance (26.7 sigma), and the discovery (4 sigma) of a 48" long X-ray tail emanating from the point source. The X-ray spectra of both the…

Astrophysics · Physics 2009-11-13 Sudip Bhattacharyya

A Chandra ACIS-S imaging observation of the nearby galaxy M81 (NGC 3031) reveals 9 luminous soft X-ray sources. The local environments, X-ray spectral properties, and X-ray light curves of the sources are presented and discussed in the…

Astrophysics · Physics 2009-11-07 Douglas Swartz , Kajal Ghosh , Valery Suleimanov , Allyn Tennant , Kinwah Wu

We present X-ray spectral analysis of 20 point-like X-ray sources detected in Chandra Planetary Nebula Survey (ChanPlaNS) observations of 59 planetary nebulae (PNe) in the solar neighborhood. Most of these 20 detections are associated with…

We present results from Chandra and XMM-Newton X-ray observations of NGC 4214, a nearby dwarf starburst galaxy containing several young regions of very active star-formation. Starburst regions are known to be associated with diffuse X-ray…

X-ray emitting diffuse nebulae around hot stars are observed to have soft-band temperatures in the narrow range [1-3]$\times10^{6}$ K, independent of the stellar wind parameters and the evolutionary stage of the central star. We discuss the…

Astrophysics of Galaxies · Physics 2018-05-16 J. A. Toalá , S. J. Arthur

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…

Solar and Stellar Astrophysics · Physics 2016-01-20 J. A. Toalá , M. A. Guerrero , Y. -H. Chu , S. J. Arthur , D. Tafoya , R. A. Gruendl

We report the Chandra detection of X-ray emission spatially coincident with the kpc-scale radio bubbles in the nearby (D_L ~ 31 Mpc) AGN-starburst galaxy NGC 6764. The X-ray emission originates in hot gas (kT ~ 0.75 keV), which may either…

Astrophysics · Physics 2009-11-13 J. H. Croston , M. J. Hardcastle , P. Kharb , R. P. Kraft , A. Hota

In this work we report spectrophotometric observations of a planetary nebula sample towards the galactic bulge. A total of 45 PNe was observed and their physical parameters (electron density and temperature) were derived. Ionic abundances…

Astrophysics · Physics 2009-11-07 A. V. Escudero , R. D. D. Costa