activity
20022025
most citedThe Conspicuous Absence of X-ray Emission from Carbon-Enriched Wolf-Rayet Stars

75 citations · 350 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2025

Chandra/HETG and NuSTAR Observations of V750 Ara, a Cas-type Star

David P. Huenemoerder, Sean J. Gunderson, Richard Ignace +6

We present 197 ks HETG and 95 ks NuSTAR spectra of the Cas-type object V750 Ara. The high-resolution X-ray spectra show that the target is similar to other objects of this cla…

astro-ph.SR2024

The Nature of X-Rays from Young Stellar Objects in the Orion Nebula Cluster -- A Chandra HETGS Legacy Project

Norbert S. Schulz, David P. Huenemoerder, David A. Principe +10

The Orion Nebula Cluster (ONC) is the closest site of very young ( 1 Myrs) massive star formation. The ONC hosts more than 1600 young and X-ray bright stars with masses rangi…

astro-ph.SR2024

Chandra HETG X-ray Spectra and Variability of Aqr, a Cas-type Be star

David P. Huenemoerder, Pragati Pradhan, Claude R. Canizares +7

High-resolution X-ray spectra of Aqr, a Cas-type star, obtained with the Chandra/HETG grating spectrometer, revealed emission lines of H-like ions of Mg, Si, S, and Fe, a…

astro-ph.HE2023

Firmamento: a multi-messenger astronomy tool for citizen and professional scientists

Dhurba Tripathi, Paolo Giommi, Adriano Di Giovanni +12

Firmamento (https://firmamento.hosting.nyu.edu) is a new-concept web-based and mobile-friendly data analysis tool dedicated to multi-frequency/multi-messenger emitters, as exemplif…

astro-ph.SR2023

Survey of X-rays from Massive Stars Observed at High Spectral Resolution with Chandra

Pragati Pradhan, David P. Huenemoerder, Richard Ignace +2

Identifying trends between observational data and the range of physical parameters of massive stars is a critical step to the still-elusive full understanding of the source, struct…

astro-ph.SR2015★ 24 cited

Probing Wolf-Rayet Winds: Chandra/HETG X-Ray Spectra of WR 6

David P. Huenemoerder, Kenneth G. Gayley, Wolf-Rainer Hamann +6

With a deep Chandra/HETGS exposure of WR 6, we have resolved emission lines whose profiles show that the X-rays originate from a uniformly expanding spherical wind of high X-ray-co…