Evidence map›Paper›PMID 39282476›Full record

ArticleNature astronomy2024

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

Stefano Facchini, Leonardo Testi, Elizabeth Humphreys, Mathieu Vander Donckt, Andrea Isella, Ramon Wrzosek, Alain Baudry, Malcom D Gray, Anita M S Richards, Wouter Vlemmings

Abstract read
In one paragraph

Article in Nature astronomy, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.

0numbers the graph read from it
0cells of the map it votes in
2citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

2 citing papers in PubMed.

  1. Article
  2. Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

10 authors.

Stefano FacchiniDipartimento di Fisica, Università degli Studi di Milano, Milano, Italy.ORCID 0000-0003-4689-2684
Leonardo TestiDipartimento di Fisica e Astronomia 'Augusto Righi', Università di Bologna, Bologna, Italy.
Elizabeth HumphreysEuropean Southern Observatory, Garching bei München, Germany.
Mathieu Vander DoncktSpace sciences, Technologies & Astrophysics Research (STAR) Institute, University of Liège, Liège, Belgium.ORCID 0000-0002-2380-6889
Andrea IsellaDepartment of Physics and Astronomy, Rice University, Houston, TX USA.ORCID 0000-0001-8061-2207
Ramon WrzosekDepartment of Physics and Astronomy, Rice University, Houston, TX USA.ORCID 0000-0002-2200-0592
Alain BaudryLaboratoire d'Astrophysique de Bordeaux, Univ. de Bordeaux, CNRS, Pessac, France.ORCID 0000-0003-1577-9427
Malcom D GrayNational Astronomical Research Institute of Thailand, Chiangmai, Thailand.ORCID 0000-0002-2094-846X
Anita M S RichardsJodrell Bank Centre for Astrophysics, University of Manchester, Manchester, UK.ORCID 0000-0002-3880-2450
Wouter VlemmingsDepartment of Space, Earth and Environment, Chalmers University of Technology, Göteborg, Sweden.ORCID 0000-0002-2700-9916

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

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 present Atacama Large Millimeter/submillimeter Array data of the ringed protoplanetary disk orbiting the young star HL Tauri that show centrally peaked, bright emission arising from three distinct transitions of the main water isotopologue (

Indexed as

Astrophysical disksEarly solar systemExoplanets

Identifiers

PMID39282476
PMCPMC11399093

What OpenQuestion holds

Textmetadata
LicenceCC BY
Read underepoch 390

Registered trials

None linked

Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.