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E. Humphreys

15 papers hereh-index 443 citations8 works total

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

author position
  • first author1
  • middle author10
  • last author2

Across the 13 of 15 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR6
  • astro-ph.EP4
  • astro-ph.GA2
  • astro-ph.IM2
  • astro-ph.HE1
same name
  • E. Humphreys — 29 papers, h 21
  • E. Humphreys — 13 papers, h 9
  • E. Humphreys — 12 papers, h 7
  • E. Humphreys — 4 papers, h 6
  • E. Humphreys — 4 papers, h 1
  • E. Humphreys — 3 papers, h 4

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
20112026
most citedFirst Results from High Angular Resolution ALMA Observations Toward the HL Tau Region

1.2k citations · 1.5k across the 13 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

astro-ph.EP2024★ 24 cited

Into the thick of it: ALMA 0.45 mm observations of HL Tau at 2 au resolution

Osmar M. Guerra-Alvarado, Carlos Carrasco-González, Enrique Macías +7

Aims. To comprehend the efficiency of dust evolution within protoplanetary disks, it is crucial to conduct studies of these disks using high-resolution observations at multiple wav…

astro-ph.EP2024★ 21 cited

Resolved ALMA observations of water in the inner astronomical units of the HL Tau disk

Stefano Facchini, Leonardo Testi, Elizabeth Humphreys +7

The water molecule is a key ingredient in the formation of planetary systems, with the water snowline being a favourable location for the growth of massive planetary cores. Here we…

astro-ph.GA2024

Sub-Parsec-Scale Jet-Driven Water Maser with Possible Gravitational Acceleration in the Radio Galaxy NGC 1052

Seiji Kameno, Yuichi Harikane, Satoko Sawada-Satoh +5

We report sub-pc-scale observations of the 321-GHz H2​O emission line in the radio galaxy NGC 1052. The H2​O line emitter size is constrained in <0.6 milliarcsec distributed…

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