Properties (45)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:associatedWith |
massive star progenitor
|
| gptkbp:bombLoad |
2004-07-29
|
| gptkbp:classification |
classified as a Type II-P supernova
|
| gptkbp:collaborations |
involved multiple international collaborations
|
| gptkbp:colors |
0.0007
|
| gptkbp:conservationEfforts |
remnant is still visible
|
| gptkbp:dataUsage |
data published in scientific journals
|
| gptkbp:education |
used in educational contexts
|
| gptkbp:energyEfficiency |
approximately 10^51 ergs
|
| gptkbp:established |
gptkb:P._A._Mazzali
|
| gptkbp:firstGeneration |
estimated progenitor mass of 8-15 solar masses
|
| gptkbp:fuelType |
core-collapse supernova
estimated explosion energy of 1-3 x 10^51 ergs |
| gptkbp:hasVolunteers |
part of larger observational campaigns
|
| gptkbp:historicalContext |
part of the historical context of supernova studies
|
| gptkbp:historicalResearch |
inspired collaborative research efforts
paved the way for future research on supernovae. |
| gptkbp:hosts |
NGC 2403
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 2004dj
|
| gptkbp:iceClass |
no significant afterglow detected
|
| gptkbp:impact |
contributed to understanding of supernovae
|
| gptkbp:internationalClassification |
provided insights into explosion dynamics
|
| gptkbp:length |
3.2 million light-years
|
| gptkbp:lighting |
analyzed for physical parameters
duration of several months plateau light curve showed a plateau phase used to estimate parameters |
| gptkbp:model |
tested various theoretical models of supernovae
|
| gptkbp:officialResidence |
data collected in multiple wavelengths
utilized advanced observational techniques |
| gptkbp:photography |
extensive photometric observations conducted
|
| gptkbp:publicAccess |
generated public interest in astronomy
|
| gptkbp:relatedEvent |
conducted by various observatories
|
| gptkbp:releaseYear |
2004-07-29
|
| gptkbp:researchInterest |
significant impact on astrophysics research
|
| gptkbp:resolution |
about 10^42 erg/s
|
| gptkbp:scientificName |
produced heavy elements
|
| gptkbp:type |
Hydrogen-rich spectrum
Type II-P supernova remnant is a neutron star or black hole |
| gptkbp:unitAwards |
maximum magnitude of about 15.5
|
| gptkbp:universe |
provides insights into cosmic distances
|
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|