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Latest Details
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| Name |
PQ Mus |
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| AAVSO UID |
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| Constellation |
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| J2000.0 |
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| B1950.0 |
12 40 38.69 -64 32 32.2 |
| Galactic coord. |
302.102 -1.957 |
Other names
(Internal only)
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Please note that aliases shown in grey link to obsolete records.
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2MASS J12433824-6448575 |
AN 102.1932 |
ASAS J124339-6449.0 |
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ASASSN-V J124338.41-644857.7 |
GDS_J1243381-644857 |
GDS_J1243394-644856 |
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HV 8464 |
IRAS 12406-6432 |
NSV 5892 |
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OGLE-GD-LPV-003092 |
OGLE-IV GD1297.11.33208 |
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| Variability type |
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M |
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| Spectral type |
M9 |
| Mag. range |
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13.5 - <16.3 V |
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| Discoverer |
-- |
| Epoch |
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| Outburst |
-- |
| Period |
445 d |
| Rise/eclipse dur. |
-- |
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Remarks
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Some references may be clicked to view in new window. Roll over index number to view submission details.
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1 |
Otero, Sebastian Alberto
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ASAS-3 magnitudes contaminated by UCAC4 126-072876 (V= 16.0; sep. 8") and UCAC4 126-072865 (V= 16.5; sep. 12"). Range has been corrected. |
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References
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Click reference title/citation to view in new window. Roll over index number to view submission details.
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1 |
Iwanek, P.; et al., 2022, The OGLE Collection of Variable Stars: Nearly
66,000 Mira Stars in the Milky Way |
2022ApJS..260...46I |
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2 |
M. Hackstein, Ch. Fein, M. Haas et al., 2015, AN 336, 590 |
2015AN....336..590H |
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3 |
E.V. Kazarovets, N.N. Samus, O.V. Durlevich, N.N. Kireeva, E.N. Pastukhova,
2008, IBVS 5863 |
2008IBVS.5863....1K |
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Pojmanski, G., 2002, The All Sky Automated Survey |
2002AcA....52..397P |
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Catalogue of Stellar Spectral Classifications (Skiff, 2009-2016) |
1993yCat.3170....0M |
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6 |
W.J.Luyten, Minn Publ 2, No.6, 1938. |
1938POMin...6....1L |
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External Links
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Location
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Catalog Data
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Information from selected catalogs obtained by cross-matching to 2 arc seconds using the CDS X-Match Service. These data may not be complete.
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2MASS
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J = 5.54 | H = 4.70 | K = 4.08 | J - K = 1.46 |
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AllWISE
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W1 = 3.16 | W2 = 2.71 | W3 = 1.50 | W4 = 0.60 | W1 - W2 = 0.46 | W3 - W4 = 0.91 |
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APASS-DR9
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B = 15.83 | V = 14.03 | g' = 15.18 | r' = 12.57 | B - V = 1.80 |
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Images
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Supporting Documents
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Revision History
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