Statements (87)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:open_cluster
|
| gptkbp:age |
approximately 100 million years
approximately 30 million years |
| gptkbp:apparent_magnitude |
6.5
7.5 used for analysis |
| gptkbp:archaeological_findings |
noted by various astronomers
|
| gptkbp:astrophysical_importance |
helps understand stellar evolution
|
| gptkbp:base_notes |
best viewed in southern hemisphere
|
| gptkbp:cluster_age_estimation |
based on stellar evolution models
|
| gptkbp:cluster_chemical_composition |
analyzed for metallicity
|
| gptkbp:cluster_dynamics_modeling |
used for simulations.
|
| gptkbp:cluster_dynamics_research |
ongoing in astrophysics community
|
| gptkbp:cluster_evolution |
monitored over time
|
| gptkbp:cluster_formation |
formed from gas and dust
|
| gptkbp:cluster_mass_estimation |
based on stellar counts
|
| gptkbp:cluster_observational_data |
available from various observatories
|
| gptkbp:cluster_structure |
loosely bound structure
|
| gptkbp:contains_star |
gptkb:NGC_3293
yes several hundred stars ongoing star formation multiple blue supergiants studied for star interactions |
| gptkbp:coordinates |
RA 11h 35m 36s, Dec -60° 24' 00"
l = 284.5°, b = -6.2° |
| gptkbp:criteria |
stars within a certain distance
|
| gptkbp:declination |
-60° 24' 00"
|
| gptkbp:diameter |
approximately 10 light years
approximately 20 light years |
| gptkbp:discovered_by |
gptkb:John_Frederick_William_Herschel
|
| gptkbp:discovery_year |
1834
|
| gptkbp:distance |
based on parallax measurements
|
| gptkbp:distance_from_earth |
approximately 4,000 light years
approximately 4,500 light years |
| gptkbp:exhibition |
gptkb:New_General_Catalogue
|
| gptkbp:has_color |
0.5
B-V = 0.3 |
| gptkbp:has_luminosity |
estimated using isochrone fitting
observed among cluster members provides insights into cluster dynamics studied for variable star populations |
| gptkbp:has_member_stars |
over 100 stars
|
| gptkbp:has_spectral_type |
various types
O and B type stars |
| gptkbp:historical_significance |
notable for its bright stars
|
| https://www.w3.org/2000/01/rdf-schema#label |
NGC 3766
|
| gptkbp:is_associated_with |
star formation regions
|
| gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
|
| gptkbp:is_part_of |
gptkb:Carina-Sagittarius_Arm
gptkb:Milky_Way_galaxy |
| gptkbp:is_studied_in |
stellar evolution research
|
| gptkbp:is_visible_from |
Southern Hemisphere
visible to the naked eye |
| gptkbp:known_as |
C 1100-610
|
| gptkbp:lighting |
analyzed for variable stars
|
| gptkbp:located_in |
gptkb:Carina_constellation
|
| gptkbp:mass |
includes main sequence stars
total mass estimated in solar masses |
| gptkbp:membership |
young stars
|
| gptkbp:membership_fraction |
high fraction of blue stars
|
| gptkbp:metallicity |
yes
|
| gptkbp:orbit_type |
none known
|
| gptkbp:photometric_analysis |
conducted for star classification
|
| gptkbp:population_density |
moderate density
|
| gptkbp:research |
documented in various catalogs
binoculars or small telescope light pollution affects visibility used to study stellar composition |
| gptkbp:research_interest |
attracts amateur astronomers
|
| gptkbp:right_ascension |
11h 35m 36s
|
| gptkbp:size |
about 10 arcminutes in diameter
|
| gptkbp:stellar_formation_history |
documented in research papers
|
| gptkbp:stellar_formation_rate |
estimated from star counts
|
| gptkbp:stellar_kinematics |
studied for motion patterns
|
| gptkbp:stellar_mass_function |
analyzed for distribution of masses
|
| gptkbp:stellar_nucleosynthesis |
investigated in cluster stars
|
| gptkbp:stellar_outflows |
studied for mass loss rates
|
| gptkbp:stellar_population_analysis |
conducted for understanding evolution
|
| gptkbp:stellar_population_synthesis |
used for modeling cluster properties
|
| gptkbp:stellar_wind_effects |
analyzed for impact on cluster dynamics
|
| gptkbp:storage |
available from various surveys
available from space telescopes |
| gptkbp:type |
Galactic open cluster
|
| gptkbp:bfsParent |
gptkb:Centaurus
gptkb:Carina_constellation |
| gptkbp:bfsLayer |
5
|