MWC 922
star in the constellation Serpens
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MWC 922
Summary
MWC 922 is a B[e]-type star[1].
Key Facts
- MWC 922's instance of is recorded as B[e]-type star[2].
- MWC 922's instance of is recorded as infrared source[3].
- MWC 922's constellation is recorded as Serpens[4].
- MWC 922's spectral class is recorded as B[e][5].
- MWC 922's catalog code is recorded as UCAC2 27151492[6].
- MWC 922's catalog code is recorded as AKARI-FIS-V1 J1821157-130139[7].
- MWC 922's catalog code is recorded as AP J18211606-1301256[8].
- MWC 922's catalog code is recorded as MWC 922[9].
- MWC 922's catalog code is recorded as Hen 3-1680[10].
- MWC 922's catalog code is recorded as IRAS 18184-1302[11].
- MWC 922's catalog code is recorded as JP11 5221[12].
- MWC 922's catalog code is recorded as 2MASS J18211606-1301256[13].
- MWC 922's catalog code is recorded as RAFGL 2132[14].
- MWC 922's catalog code is recorded as SS73 156[15].
- MWC 922's catalog code is recorded as TIC 117193899[16].
- MWC 922's catalog code is recorded as UCAC4 385-101175[17].
- MWC 922's catalog code is recorded as WISE J182116.01-130124.6[18].
- MWC 922's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.80'}[19].
- MWC 922's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.65'}[20].
- MWC 922's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.412303'}[21].
- MWC 922's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.960'}[22].
- MWC 922's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.396'}[23].
- MWC 922's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.704'}[24].
- MWC 922's has effect is recorded as Red Square Nebula[25].
- MWC 922's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-497.756989'}[26].
Body
Designation and Status
Recorded instance of include B[e]-type star[2] and infrared source[3].
History and Context
Catalog codes include UCAC2 27151492[6], AKARI-FIS-V1 J1821157-130139[7], AP J18211606-1301256[8], MWC 922[9], Hen 3-1680[10], and IRAS 18184-1302[11].