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Research draft

protostar

vr.tr.protostar · PHY.SPC

Let an agent describe protostars by stage, host cloud, observations and theory of star formation, with sourced data.

Thing Registry Physical world and living systems

Research draft, second pass

A second pass drafted this model: the structure a model of this thing needs, and what is known about it in the world. The line under this one says how the second half was obtained - researched against sources, or recalled without web access, in which case nothing here was read anywhere and every claim is a lead to verify. Unreviewed either way.

written by Claude from model knowledge without web access - no source was read, every claim is a lead to verify

Researched by: Claude

Purpose and description

Let an agent describe protostars by stage, host cloud, observations and theory of star formation, with sourced data.

A very young star still gathering mass from its parent molecular cloud, before hydrogen fusion begins in its core; protostars are hidden in dusty envelopes and observed mainly in infrared and radio.

What it is for: Understanding how stars and planetary systems form.

It can be explain protostellar stages; find observations in infrared and radio; relate protostars to outflows and disks; compare with pre-main-sequence stars.

Distinguishing features

Still accreting mass

No core hydrogen fusion yet

Embedded in envelopes

Short-lived stage

What it looks like

Hidden in dust; seen as infrared sources with jets and outflows.

How it is recognised

Class 0 and Class I sources

Bipolar outflows and Herbig-Haro objects

T Tauri stars are a later stage

Related models

is a kind of - category

young stellar object

forms in - birthplace

molecular cloud

is surrounded by - structure

protoplanetary disk

becomes - next stage

pre-main-sequence star

In practice

Families and kinds

Class 0 protostars

Class I protostars

low-mass protostars

massive protostars

Failure modes and hazards

Overstating certainty of stage classification

Presenting processed images without notes

Where this came from

wikidata · CC0 1.0

Drafted structure

Bundle to layer to finding to question, as the second pass will find it: 4 bundles · 8 layers · 8 findings · 16 questions.

Object Which protostar.

Catalogues identify.

Identity

Designation.

Identity

Designation.

  1. Which protostar is meant, in which cloud? provenance
  2. Which catalogue lists it? provenance

Stage

Class.

Stage

Evolutionary stage.

  1. What evolutionary class is it assigned? provenance
  2. On what evidence? boundary
Observation Telescopes.

Infrared and radio reveal protostars.

Instruments

Wavelengths.

Instruments

Instruments.

  1. Which telescopes and wavelengths observed it? provenance
  2. What features were seen? provenance

Outflows

Jets.

Outflows

Outflows.

  1. Does it drive jets or outflows? provenance
  2. How were they measured? measurement
Physics Formation.

Theory explains formation.

Accretion

Mass growth.

Accretion

Accretion.

  1. How fast is it accreting mass, according to studies? measurement
  2. How uncertain is it? boundary

Future

Final mass.

Future

Future evolution.

  1. What kind of star is it expected to become? provenance
  2. Based on which models? provenance
Teaching Explaining.

Clear explanations help.

Explain

Simple terms.

Explain

Explanation.

  1. How can star formation be explained simply? action
  2. Which images help? provenance

Images

Processing.

Images

Image processing.

  1. Are colours in the image representative or mapped? boundary
  2. Who processed it? provenance

What the second pass must settle

  • Should stages be separate entries?
  • How should survey catalogues be linked?
  • How should massive star formation be handled?