Statements (53)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Taurus
|
| gptkbp:are_less_active_than |
classical T Tauri stars
|
| gptkbp:are_less_bright_than |
more evolved stars
|
| gptkbp:are_less_common_than |
classical T Tauri stars
|
| gptkbp:are_less_luminous_than |
classical T Tauri stars
|
| gptkbp:are_less_massive_than |
more massive stars
|
| gptkbp:are_often_investigated_for |
their magnetic fields
|
| gptkbp:are_part_of |
the Gould Belt
the Taurus-Auriga star-forming region |
| gptkbp:are_typically_found_in |
regions of active star formation
|
| gptkbp:are_typically_located_in |
star-forming regions
|
| gptkbp:are_typically_younger_than |
10 million years
|
| gptkbp:are_younger_than |
1 million years
|
| gptkbp:associated_with |
star formation regions
|
| gptkbp:can_be_found_in |
star clusters
the Chamaeleon complex |
| gptkbp:can_detect |
infrared observations
|
| gptkbp:can_exhibit_variability_in |
brightness over time
|
| gptkbp:characterized_by |
weak emission lines
|
| gptkbp:exhibits |
accretion processes
variable luminosity outflows and jets disk accretion phenomena spectral variability. |
| gptkbp:has_spectral_type |
K to M type
|
| gptkbp:have_mass_range |
0.1 to 2 solar masses
|
| https://www.w3.org/2000/01/rdf-schema#label |
Weak-line T Tauri stars
|
| gptkbp:is_considered_to_be |
low-mass stars
the earliest stage of stellar evolution |
| gptkbp:is_essential_for |
studying stellar evolution
stellar magnetic activity the initial mass function understanding the formation of planetary systems |
| gptkbp:is_found_in |
the Orion Nebula
the Lupus star-forming region |
| gptkbp:is_monitored_by |
changes in spectral lines
|
| gptkbp:is_often_associated_with |
gptkb:Herbig-Haro_objects
young stellar objects |
| gptkbp:is_often_seen_in |
molecular clouds
the Scorpius-Centaurus association |
| gptkbp:is_often_used_in |
probes of star formation
|
| gptkbp:is_recognized_by |
their spectral characteristics
their low luminosity |
| gptkbp:is_studied_for |
planet formation processes
|
| gptkbp:is_studied_in |
gptkb:spectroscopy
astrophysics photometry the context of star formation theory |
| gptkbp:may_have |
protoplanetary disks
circumstellar material |
| gptkbp:type_of |
pre-main-sequence stars
|
| gptkbp:bfsParent |
gptkb:Taurus
|
| gptkbp:bfsLayer |
5
|