Properties (47)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:associatedWith |
cosmological measurements
|
| gptkbp:collaboratedWith |
collaborated with various observatories
|
| gptkbp:collaborations |
involved many international astronomers
|
| gptkbp:colors |
0.0055
|
| gptkbp:conservationEfforts |
remnant is still being studied
|
| gptkbp:contributedTo |
contributed to the understanding of dark energy
|
| gptkbp:dataUsage |
data published in numerous scientific journals
|
| gptkbp:education |
educational value in astronomy courses
|
| gptkbp:established |
gptkb:Robert_Kirshner
|
| gptkbp:fuelType |
approximately 1.2 x 10^51 ergs
|
| gptkbp:generator |
likely a white dwarf star
|
| gptkbp:historicalSignificance |
historically significant for Type Ia supernova research
|
| gptkbp:hosts |
part_of_the_Virgo_constellation
|
| https://www.w3.org/2000/01/rdf-schema#label |
SN 1991T
|
| gptkbp:image |
photometric data analyzed extensively
|
| gptkbp:impact |
impact on the study of the expansion of the universe
|
| gptkbp:internationalClassification |
spectroscopy revealed chemical composition
|
| gptkbp:legacy |
legacy continues in modern astrophysics research
|
| gptkbp:length |
approximately 60 million light-years from Earth
|
| gptkbp:lighting |
similar to other Type Ia supernovae
light curve shows a rapid rise and decline reached peak brightness within 20 days used for cosmological distance measurements light curve analysis supports the standard candle model |
| gptkbp:lightRange |
light curve template used for comparison
|
| gptkbp:locatedIn |
galaxy NGC 4526
|
| gptkbp:model |
used to test theoretical models of supernovae
|
| gptkbp:notableFeature |
notable for its brightness and early rise
|
| gptkbp:occursAnnually |
important for understanding Type Ia supernovae
|
| gptkbp:officialResidence |
data collected from various telescopes
utilized advanced observational techniques |
| gptkbp:publicAccess |
generated public interest in supernovae
|
| gptkbp:reduces |
declined at a rate typical for Type Ia supernovae
|
| gptkbp:relatedEvent |
follow-up observations continue to this day
follow-up studies have provided insights into supernova mechanics |
| gptkbp:releaseYear |
1991-02-24
in_the_constellation_Virgo |
| gptkbp:researchInterest |
significant impact on astrophysics research
|
| gptkbp:scientificName |
widely discussed in the scientific community
|
| gptkbp:thematicElement |
spectral features indicate rapid expansion
|
| gptkbp:type |
gptkb:Type_Ia_supernova
remnant is a nebula shows features of both iron and silicon |
| gptkbp:unitAwards |
maximum magnitude of about -19.5
|
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
multiple wavelengths including optical and infrared |