◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

J. Eisner

58 papers hereh-index 282.1k citations81 works total

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

author position
  • sole author2
  • first author6
  • middle author37
  • last author11

Across the 56 of 58 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR20
  • astro-ph.EP17
  • astro-ph10
  • astro-ph.IM7
  • astro-ph.GA4
same name
  • J. Eisner — 10 papers, h 3
  • J. Eisner — 8 papers, h 6
  • J. Eisner — 4 papers, h 2
  • J. Eisner — 2 papers, h 1

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
20012024
most citedAccreting Protoplanets in the LkCa 15 Transition Disk

302 citations · 2.8k across the 58 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.SRShow all

4 papers · 2 filters

astro-ph.SR2017★ 64 cited

Disk Masses for Embedded Class I Protostars in the Taurus Molecular Cloud

Patrick D. Sheehan, Josh A. Eisner

Class I protostars are thought to represent an early stage in the lifetime of protoplanetary disks, when they are still embedded in their natal envelope. Here we measure the disk m…

astro-ph.SR2017★ 10 cited

Improved Constraints on the Disk Around MWC 349A from the 23-Meter LBTI

Steph Sallum, Josh Eisner, Phil Hinz +4

We present new spatially resolved observations of MWC 349A from the Large Binocular Telescope Interferometer (LBTI), a 23-meter baseline interferometer made up of two, co-mounted 8…

astro-ph.SR2017★ 53 cited

WL 17: A Young Embedded Transition Disk

Patrick D. Sheehan, Josh A. Eisner

We present the highest spatial resolution ALMA observations to date of the Class I protostar WL 17 in the ρ Ophiuchus L1688 molecular cloud complex, which show that it has a 12 A…

astro-ph.SR2017★ 96 cited

The ALMA View of the OMC1 Explosion in Orion

John Bally, Adam Ginsburg, Hector Arce +4

Most massive stars form in dense clusters where gravitational interactions with other stars may be common. The two nearest forming massive stars, the BN object and Source I, locate…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.