most citedThe Chandra Planetary Nebulae Survey (ChanPlaNS): III. X-ray Emission from the Central Stars of Planetary Nebulae

68 citations · 169 across the 6 of their papers we have counts for

collaborators

9 papers

astro-ph.IM20231 cited

The life cycle of stars and their planets from the high energy perspective

Lia Corrales, Keivan G. Stassun, Tim Cunningham +19

One of the key research themes identified by the Astro2020 decadal survey is Worlds and Suns in Context. The Advanced X-ray Imaging Satellite (AXIS) is a proposed NASA APEX mission…

astro-ph.SR2023

Discovery of Radial Spectral Hardening in the Hot Bubble of Planetary Nebula BD+30 3639 with Median Energy Imaging

Rodolfo Montez

We introduce a new imaging analysis technique to study the spatial distribution of the X-ray emission from the hot bubble of planetary nebula BD+30 3639. Hot bubble emission is typ…

astro-ph.HE202314 cited

Peering into the central region of a nano-quasar: XMM-Newton and Chandra views of the CH Cyg Symbiotic System

J. A. Toalá, O. González-Martín, M. Karovska +3

We present the analysis of archival XMM-Newton and Chandra observations of CH Cyg, one of the most studied symbiotic stars (SySts). The combination of the high-resolution XMM-Newto…

astro-ph.SR20237 cited

Shocks and Photoionization of the Inner 650 AU Jet of the Interacting Binary Star R Aquarii from Multiwavelength Hubble Space Telescope Observations

Caroline D. Huang, Margarita Karovska, Warren Hack +3

Astrophysical jets are present in a range of environments, including young stellar objects, X-ray binaries, and active galactic nuclei, but their formation is still not fully under…

astro-ph.SR2023

The messy death of a multiple star system and the resulting planetary nebula as observed by JWST

Orsola De Marco, Muhammad Akashi, Stavros Akras +66

Planetary nebulae (PNe), the ejected envelopes of red giant stars, provide us with a history of the last, mass-losing phases of 90 percent of stars initially more massive than the…

astro-ph.SR201411 cited

Constraints on the Surface Magnetic Fields and Age of a Cool Hypergiant: XMM-Newton X-ray Observations of VY CMa

R. Montez, J. H. Kastner, R. M. Humphreys +2

The complex circumstellar ejecta of highly evolved, cool hypergiants are indicative of multiple, asymmetric mass loss events. To explore whether such episodic, non-isotropic mass l…