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20112026
most citedPulsar Wind Nebulae Created by Fast-Moving Pulsars

84 citations · 544 across the 26 of their papers we have counts for

collaborators

27 papers

astro-ph.HE2026

XClass: An Automated Multiwavelength Machine-Learning Pipeline for Classification of Extragalactic X-ray Sources. I. Pipeline Description

Blagoy Rangelov, Nicholas Moore, Haley Dutton +1

Most X-ray sources detected in nearby galaxies by the Chandra X-ray Observatory lack astrophysical classifications. We present XClass (X-ray Classifier for extragalactic sources),…

astro-ph.HE2025★ 1 cited

Neutron star heating vs. HST observations

Luis E. Rodríguez, Andreas Reisenegger, Denis González-Caniulef +5

Passively cooling neutron stars (NSs) should reach undetectably low surface temperatures K in less than yr. However, HST observations have revealed likely thermal…

astro-ph.HE2023

A VLITE Search for Millisecond Pulsars in Globular Clusters: Discovery of a Pulsar in GLIMPSE-C01

Amaris V. McCarver, Thomas J. Maccarone, Scott M. Ransom +8

We present results from a search for pulsars in globular clusters, including the discovery of a new millisecond pulsar in the stellar cluster GLIMPSE-C01. We searched for low frequ…

astro-ph.HE2023★ 4 cited

Chandra X-ray Observatory Observations of 13 Fermi LAT Sources

Blagoy Rangelov, Hui Yang, Brice Williams +3

In the latest data release from the Fermi -ray Space Telescope (the 4th Fermi LAT 14 yr Catalog, or 4FGL), more than 50% of the Galactic sources are yet to be identified. We obs…

astro-ph.HE2022★ 6 cited

Population of X-ray Sources in the Intermediate-Age Cluster NGC 3532: a Test Bed for Machine-Learning Classification

Steven Chen, Oleg Kargaltsev, Hui Yang +4

Open clusters are thought to be the birth place of most stars in the Galaxy. Thus, they are excellent laboratories for investigating stellar evolution, and X-ray properties of vari…

astro-ph.HE2022★ 32 cited

Classifying Unidentified X-ray Sources in the Chandra Source Catalog Using a Multiwavelength Machine-learning Approach

Hui Yang, Jeremy Hare, Oleg Kargaltsev +3

The rapid increase in serendipitous X-ray source detections requires the development of novel approaches to efficiently explore the nature of X-ray sources. If even a fraction of t…

astro-ph.HE2021★ 5 cited

X-ray binaries in M51 I: catalog and statistics

Jared R. Rice, Blagoy Rangelov, Andrea Prestwich +3

We used archival data from the \emph{Chandra X-ray Observatory} (\emph{Chandra}) and the \emph{Hubble Space Telescope}, to identify 334 candidate X-ray binary (XRB) systems and the…

astro-ph.HE2019★ 5 cited

Runaway O-star Bow Shocks as Particle Accelerators? The Case of AE Aur revisited

Blagoy Rangelov, Thierry Montmerle, S. R. Federman +2

We present results of our Chandra/ACIS observations of the field centered on the fast, runaway O star AE Aur and its bow shock. Previous XMM-Newton observations revealed an X-ray "…

astro-ph.HE2019★ 4 cited

XMM-Newton and Chandra observations of the unidentified Fermi-LAT source 3FGL J1016.5-6034: A Young Pulsar with a Nebula?

Jeremy Hare, Igor Volkov, Oleg Kargaltsev +2

We report the discovery of a bright X-ray source in the XMM-Newton and Chandra X-ray Observatory (CXO) images of the unidentified Fermi-LAT source 3FGL J1016.5-6034. The XMM-Newton…

astro-ph.HE2019★ 51 cited

Hubble Space Telescope non-detection of PSR J2144-3933: the coldest known neutron star

S. Guillot, G. G. Pavlov, C. Reyes +4

We report non-detections of the yr old, slow, isolated, rotation-powered pulsar PSR J21443933 in observations with the Hubble Space Telescope in one optical…

astro-ph.HE2018★ 20 cited

A long hard-X-ray look at the dual active galactic nuclei of M51 with NuSTAR

M. Brightman, M. Baloković, M. Koss +14

We present a broadband X-ray spectral analysis of the M51 system, including the dual active galactic nuclei (AGN) and several off-nuclear point sources. Using a deep observation by…

astro-ph.HE2017★ 41 cited

Old but still warm: Far-UV detection of PSR B0950+08

G. G. Pavlov, B. Rangelov, O. Kargaltsev +3

We report on a Hubble Space Telescope detection of the nearby, old pulsar B0950+08 ( pc, spin-down age 17.5 Myr) in two far-ultraviolet (FUV) bands. We measured the me…

astro-ph.HE2017★ 84 cited

Pulsar Wind Nebulae Created by Fast-Moving Pulsars

Oleg Kargaltsev, George G. Pavlov, Noel Klingler +1

We review multiwavelength properties of pulsar wind nebulae (PWNe) created by supersonically moving pulsars and the effects of pulsar motion on the PWN morphologies and the ambient…

astro-ph.HE2017★ 8 cited

Chandra Observations of the field containing HESS J1616-508

Jeremy Hare, Oleg Kargaltsev, George G. Pavlov +2

We report the results of three Chandra observations covering most of the extent of the TeV gamma-ray source HESS J1616-508 and a search for a lower energy counterpart to this sourc…

astro-ph.HE2017★ 13 cited

CTIO, ROSAT HRI and Chandra ACIS Observations of the Archetypical Mixed-Morphology Supernova Remnant W28 (G6.4-0.1)

Thomas G. Pannuti, Jeonghee Rho, Oleg Kargaltsev +6

We present a joint analysis of optical emission-line and X-ray observations of the archetypical Galactic mixed-morphology supernova remnant (MMSNR) W28 (G6.4-0.1). MMSNRs comprise…

astro-ph.HE2017★ 56 cited

Hubble Space Telescope detection of the millisecond pulsar J2124-3358 and its far-ultraviolet bow shock nebula

B. Rangelov, G. G. Pavlov, O. Kargaltsev +4

We observed a nearby millisecond pulsar J2124-3358 with the Hubble Space Telescope in broad far-UV (FUV) and optical filters. The pulsar is detected in both bands with fluxes F(125…

astro-ph.HE2016★ 38 cited

Deep Chandra Observations of the Pulsar Wind Nebula Created by PSR B0355+54

Noel Klingler, Blagoy Rangelov, Oleg Kargaltsev +10

We report on Chandra X-ray Observatory (CXO) observations of the pulsar wind nebula (PWN) associated with PSR B0355+54 (eight observations with a 395 ks total exposure, performed o…

astro-ph.HE2016★ 26 cited

First Detection of a Pulsar Bow Shock Nebula in Far-UV: PSR J0437-4715

Blagoy Rangelov, George G. Pavlov, Oleg Kargaltsev +3

Pulsars traveling at supersonic speeds are often accompanied by cometary bow shocks seen in Halpha. We report on the first detection of a pulsar bow shock in the far-ultraviolet (F…

astro-ph.HE2016★ 42 cited

Chandra Observations of Outflows from PSR J1509-5850

Noel Klingler, Oleg Kargaltsev, Blagoy Rangelov +3

PSR J1509-5850 is a middle-aged pulsar with the period P ~ 89 ms, spin-down power Edot = 5.1 x 10^35 erg/s, at a distance of about 3.8 kpc. We report on deep Chandra X-ray Observat…

astro-ph.HE2015★ 12 cited

Magnesium-rich Ejecta in the SNR G284.31.8 Around the High-Mass Gamma-Ray Binary 1FGL J1018.65856

Brian J. Williams, Blagoy Rangelov, Oleg Kargaltsev +1

We present results from two {\it Chandra} observations of the 16.6 d X-ray/-ray high-mass binary 1FGL J1018.65856 located at the center of the supernova remnant G284.31.8.…

astro-ph.HE2015★ 11 cited

Multi-wavelength study of HESS J1741-302

Jeremy Hare, Blagoy Rangelov, Eda Sonbas +1

We present the results of two Chandra X-ray Observatory ( CXO) observations of TeV gamma-ray source HESS J1741-302A/B. Our analysis also includes GeV gamma-ray and radio data. We i…

astro-ph.HE2015

An extended X-ray object ejected from the PSR B1259-63/LS 2883 binary

George G. Pavlov, Jeremy Hare, Oleg Kargaltsev +2

We present the analysis of the Chandra X-ray Observatory observations of the eccentric gamma-ray binary PSR B1259-63/LS 2883. The analysis shows that the extended X-ray feature see…

astro-ph.HE2014★ 6 cited

Multiwavelength study of the northeastern outskirts of the extended TeV source HESS J1809-193

Blagoy Rangelov, Bettina Posselt, Oleg Kargaltsev +3

HESS J1809-193 is an extended TeV gamma-ray source in the Galactic Plane. Multiwavelength observations of the HESS J1809-193 field reveal a complex picture. We present results from…

astro-ph.HE2013★ 10 cited

Chandra Imaging of Gamma-Ray Binaries

Oleg Kargaltsev, Blagoy Rangelov, Jeremy Hare +1

We review the multiwavelength properties of the few known gamma-ray binaries, focusing on extended emission recently resolved with Chandra. We discuss the implications of these fin…