Statements (57)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:nebula
|
| gptkbp:bfsLayer |
5
|
| gptkbp:bfsParent |
gptkb:GRB_031203
|
| gptkbp:apparent_magnitude |
maximum magnitude of approximately -17.5
|
| gptkbp:archives |
data archived for future reference
|
| gptkbp:bomb_load |
likely due to core collapse of a massive star
|
| gptkbp:category |
designated as SN 2003lw
|
| gptkbp:collaborations |
collaboration with international astronomers
collaborative research efforts enhanced knowledge part of a larger collaboration network |
| gptkbp:community |
contributed to the scientific community's understanding of supernovae
|
| gptkbp:community_engagement |
generated public interest in supernova research
|
| gptkbp:community_involvement |
outreach activities conducted to share findings
|
| gptkbp:composed_of |
enriched in elements like nickel and iron
|
| gptkbp:connects |
possible connection to collapsar models
|
| gptkbp:conservation_efforts |
gptkb:nebula
|
| gptkbp:discovered_by |
gptkb:L._A._A._de_Vaucouleurs
|
| gptkbp:distance |
approximately 3.2 million light-years from Earth
distance estimated using Cepheid variables |
| gptkbp:education |
educational value for astronomy students
|
| gptkbp:emissions_standard |
radio emission monitored
|
| gptkbp:events |
follow-up observations conducted by various observatories
|
| gptkbp:followed_by |
afterglow observed in various wavelengths
|
| gptkbp:future_plans |
paved the way for future research on supernovae.
|
| gptkbp:has_luminosity |
neutrino emission studied
related to stellar evolution studies |
| gptkbp:has_spectral_type |
Hydrogen-rich spectrum
|
| gptkbp:hosts |
gptkb:NGC_2403
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 2003lw
|
| gptkbp:impact |
contributed to understanding of supernova mechanisms
impact on future supernova research |
| gptkbp:legacy |
legacy of observations for future studies
|
| gptkbp:length |
around 2003-11-24
|
| gptkbp:lighting |
light curve analysis provided insights into explosion dynamics
Type II light curve X-ray emission observed post-explosion gamma-ray emission detected light curve fitting analysis performed light curve variability analyzed peaked around 20 days after explosion plateau phase observed |
| gptkbp:publishes |
data published in astronomical journals
numerous publications resulting from observations |
| gptkbp:redshift |
0.0007
|
| gptkbp:related_event |
associated with a gamma-ray burst
|
| gptkbp:related_model |
tested theoretical models of supernova explosions
|
| gptkbp:released |
released energy equivalent to about 10^51 ergs
|
| gptkbp:research |
2003 to 2004
utilized various observational techniques observed by multiple telescopes spectroscopic observations conducted |
| gptkbp:scientific_classification |
core-collapse supernova
important for supernova classification schemes |
| gptkbp:storage |
photometric observations conducted
|
| gptkbp:type |
gptkb:Type_II_supernova
|
| gptkbp:universe |
has cosmological implications for distance measurements
|
| gptkbp:year_created |
2003-11-24
|