Statements (46)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
galaxy
|
| gptkbp:colors |
0.0183
|
| gptkbp:contains |
active galactic nucleus
numerous young star clusters |
| gptkbp:culturalSignificance |
mentioned in documentaries and books
|
| gptkbp:emissionsStandard |
strong infrared emission
|
| gptkbp:features |
two colliding galaxies
|
| gptkbp:hasArea |
available images from various telescopes
|
| gptkbp:hasAudience |
important for studying galaxy evolution
|
| gptkbp:hasCitations |
difficult to observe due to brightness
influences nearby galaxies |
| gptkbp:hasCollaborationsWith |
international astronomical community
studied by multiple research teams |
| gptkbp:hasDemographics |
available photometric observations
|
| gptkbp:hasEducation |
used in astronomy education
|
| gptkbp:hasFacility |
high velocity dispersion
|
| gptkbp:hasFeature |
available spectroscopic observations
|
| gptkbp:hasFilm |
merging galaxies
|
| gptkbp:hasFuturePlans |
planned for future telescopes
|
| gptkbp:hasGoals |
detected X-ray emissions
part of the Arp 220 group two nuclei |
| gptkbp:hasHistoricalSignificance |
noted in astronomical literature
|
| gptkbp:hasLocation |
rich in dust and gas
|
| gptkbp:hasNationality |
subject of various theoretical models
|
| gptkbp:hasOccupation |
over 100 solar masses per year
|
| gptkbp:hasPublications |
numerous scientific papers published
popular target for amateur astronomers |
| gptkbp:hasRelatedPatent |
Seyfert 2
|
| gptkbp:hasResearchInterest |
ongoing research into its properties
|
| gptkbp:hasResidence |
observational astronomy
one of the brightest infrared sources |
| gptkbp:hasSibling |
about 10,000 light-years across
|
| gptkbp:hasSpecialty |
visible in optical wavelengths
|
| gptkbp:hasVariants |
strong radio source
|
| https://www.w3.org/2000/01/rdf-schema#label |
Arp 220
|
| gptkbp:isIntegratedWith |
ongoing merger process
|
| gptkbp:length |
approximately 250 million light-years
|
| gptkbp:locatedIn |
constellation_Ursa_Major
|
| gptkbp:partOf |
Arp catalog of peculiar galaxies
|
| gptkbp:releaseYear |
1975
|
| gptkbp:resolution |
about 450 times that of the Milky Way
|
| gptkbp:type |
ultra-luminous infrared galaxy
|
| gptkbp:unitAwards |
14.3
|
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|
| gptkbp:weight |
approximately 100 billion solar masses
|