Evidence map›Paper›PMID 41035786›Full record

ReviewSpace science reviews2025

The Origins & Reservoirs of Exocomets.

Michele Bannister, Susanne Pfalzner, Tim Pearce, Alexander J Mustill, Hubert Klahr, Hideko Nomura, Nagayoshi Ohashi, Rosita Kokotanekova, Sebastian Marino, Dennis Bodewits and 4 more

Abstract readReview
PubMed Full text at PMC Publisher
In one paragraph

Review in Space science reviews, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 1 paper.

0numbers the graph read from it
0cells of the map it votes in
1citing 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

1 citing paper in PubMed.

  1. The Origins & Reservoirs of Exocomets.Space science reviews · 2025
    Review
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

14 authors.

Michele BannisterSchool of Physical and Chemical Sciences - Te Kura Matū, University of Canterbury, Private Bag 4800, Christchurch, 8140 New Zealand.
Susanne PfalznerJülich Supercomputing Centre, Research Centre Jülich, Wilhelm-Johnen-Strasse, Jülich, 52428 Germany.ORCID 0000-0002-5003-4714
Tim PearceDepartment of Physics, University of Warwick, Gibbet Hill Road, Coventry, CV4 7AL United Kingdom.
Alexander J MustillDepartment of Physics, Lund University, Box 118, Lund, 22100 Sweden.
Hubert KlahrMax Planck Institut für Astronomie, Königstuhl 17, Heidelberg, 69117 Germany.
Hideko NomuraDivision of Science, National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8551 Japan.
Nagayoshi OhashiAcademia Sinica Institute of Astronomy & Astrophysics, 11F of Astronomy-Mathematics Building, AS/NTU, No.1, Sec. 4, Roosevelt Rd, Taipei, 106319 Taiwan, R.O.C.
Rosita KokotanekovaInstitute of Astronomy and NAO, Bulgarian Academy of Sciences, 72 Tsarigradsko Chaussee Blvd., Sofia, 1784 Bulgaria.
Sebastian MarinoDepartment of Physics and Astronomy, University of Exeter, Stocker Road, Exeter, EX4 4QL UK.
Dennis BodewitsDepartment of Physics, Auburn University, Edmund C. Leach Science Center, Auburn, 36849 AL USA.
Raphael MarschallLaboratoire J.-L. Lagrange, Observatoire de la Côte d'Azur, CNRS, CS 34229, Nice Cedex 4, 06304 France.
Darryl Z SeligmanDepartment of Physics and Astronomy, Michigan State University, East Lansing, 48824 MI USA.
Geraint H JonesUCL Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, RH5 6NT UK.
Dimitri VerasDepartment of Physics, University of Warwick, Gibbet Hill Road, Coventry, CV4 7AL United Kingdom.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Small bodies exist in distinct populations within their planetary systems. These reservoir populations hold a range of compositions, which to first order are dependent on formation location relative to their star. We provide a general overview of the nature of the reservoirs that source exocomets, from the influence of the stellar environment through planetesimal formation to comparisons with Solar System populations. Once transitioned from a young protoplanetary disc to a debris disc, a star can expect to be rained with exocomets. While exocomets are predominantly detected to date at A-type stars, planetesimals plausibly exist across a range of stellar masses, based on exoplanet abundance, debris disc occurrence and white dwarf infall.

Identifiers

PMID41035786
PMCPMC12479627

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.