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D. Coffey

34 papers hereh-index 161.3k citations59 works total

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

author position
  • sole author1
  • first author8
  • middle author18
  • last author1

Across the 28 of 34 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR22
  • astro-ph6
  • astro-ph.GA4
  • astro-ph.IM1
  • physics.space-ph1
same name
  • D. Coffey — 12 papers, h 6
  • D. Coffey — 8 papers, h 7
  • D. Coffey — 6 papers, h 16
  • D. Coffey — 3 papers, h 2

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
20032025
most citedRotation of Jets from Young Stars: New Clues from the Hubble Space Telescope Imaging Spectrograph

198 citations · 1.2k across the 34 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.SR2020★ 2 cited

The GRAVITY Young Stellar Object survey IV. The CO overtone emission in 51 Oph at sub-au scales

GRAVITY Collaboration, M. Koutoulaki, R. Garcia Lopez +69

51 Oph is a Herbig Ae/Be star that exhibits strong near-infrared CO ro-vibrational emission at 2.3 micron, most likely originating in the innermost regions of a circumstellar disc.…

astro-ph.SR2020

Possible Time Correlation Between Jet Ejection and Mass Accretion for RW Aur A

Michihiro Takami, Tracy L. Beck, P. Christian Schneider +17

For the active T-Taur star RW Aur A we have performed long-term (~10 yr) monitoring observations of (1) jet imaging in the [Fe II] 1.644-micron emission line using Gemini-NIFS and…

astro-ph.SR2020

Mirror, mirror on the outflow cavity wall. Near-infrared CO overtone disc emission of the high-mass YSO IRAS 11101-5829

R. Fedriani, A. Caratti o Garatti, M. Koutoulaki +7

Aims: The inner regions of high-mass protostars are often invisible in the near-infrared. We aim to investigate the inner gaseous disc of IRAS11101-5829 through scattered light fro…

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