L 326-61
high proper-motion star in the constellation Centaurus
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L 326-61
Summary
L 326-61 is a high proper-motion star[1].
Key Facts
- L 326-61's instance of is recorded as high proper-motion star[2].
- L 326-61's constellation is recorded as Centaurus[3].
- L 326-61's spectral class is recorded as M3.5:[4].
- L 326-61's catalog code is recorded as NLTT 30554[5].
- L 326-61's catalog code is recorded as Gaia DR2 6131272458806020736[6].
- L 326-61's catalog code is recorded as GJ 1157[7].
- L 326-61's catalog code is recorded as L 326-61[8].
- L 326-61's catalog code is recorded as LFT 901[9].
- L 326-61's catalog code is recorded as LHS 2552[10].
- L 326-61's catalog code is recorded as LTT 4669[11].
- L 326-61's catalog code is recorded as [RHG95] 1940[12].
- L 326-61's catalog code is recorded as 2MASS J12230147-4637082[13].
- L 326-61's catalog code is recorded as RAVE J122301.5-463708[14].
- L 326-61's catalog code is recorded as WISEA J122300.66-463712.1[15].
- L 326-61's catalog code is recorded as GCRV 26285[16].
- L 326-61's catalog code is recorded as UCAC4 217-065660[17].
- L 326-61's catalog code is recorded as PM J12230-4637[18].
- L 326-61's ARICNS is recorded as 02136[19].
- L 326-61's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.62'}[20].
- L 326-61's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.24'}[21].
- L 326-61's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.1693'}[22].
- L 326-61's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.168'}[23].
- L 326-61's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.627'}[24].
- L 326-61's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.362'}[25].
- L 326-61's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.273'}[26].
Body
Designation and Status
L 326-61's instance of is recorded as high proper-motion star[2].
History and Context
Catalog codes include NLTT 30554[5], Gaia DR2 6131272458806020736[6], GJ 1157[7], L 326-61[8], LFT 901[9], and LHS 2552[10].