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M. Eracleous

53 papers hereh-index 161.4k citations70 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author40
  • last author4

Across the 46 of 53 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA31
  • astro-ph10
  • astro-ph.HE5
  • astro-ph.CO4
  • astro-ph.SR2
  • astro-ph.IM1
same name
  • M. Eracleous — 172 papers, h 59
  • M. Eracleous — 17 papers, h 10

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19972026
most citedLarge-Amplitude X-ray Outbursts from Galactic Nuclei: A Systematic Survey Using ROSAT Archival Data

246 citations · 1.3k across the 51 of their papers we have counts for

collaborators
Showing 2023 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2023

The IRX-Beta Relation in kpc-sized Star Forming Regions in Nearby Galaxies

Laura Duffy, Mallory Molina, Michael Eracleous +7

The effect of dust attenuation on a galaxy's light depends on a number of physical properties, such as geometry and dust composition, both of which can vary across the faces of gal…

astro-ph.GA2023★ 1 cited

Panic at the ISCO: time-varying double-peaked broad lines from evolving accretion disks are common amongst optically variable AGN

Charlotte Ward, Suvi Gezari, Peter Nugent +12

About 3-10\% of Type I active galactic nuclei (AGN) have double-peaked broad Balmer lines in their optical spectra originating from the motion of gas in their accretion disk. Doubl…

astro-ph.GA2023

ReveaLLAGN 0: First Look at JWST MIRI data of Sombrero and NGC 1052

K. Goold, A. Seth, M. Molina +28

We present the first results from the Revealing Low-Luminosity Active Galactic Nuclei (ReveaLLAGN) survey, a JWST survey of seven nearby LLAGN. We focus on two observations with th…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.