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Latest Details
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| Name |
PNV J17345432-1423182 |
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| AAVSO UID |
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000-BMH-553 (No observations) |
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| Constellation |
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| J2000.0 |
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| B1950.0 |
17 32 03.65 -14 21 21.3 |
| Proper motion |
| RA: -7.6 +/- 6.2 mas/y | Dec: -8.2 +/- 6.8 mas/y | Source: UCAC4 |
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| Galactic coord. |
11.138 +9.744 |
Other names
(Internal only)
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2MASS J17345436-1423172 |
ASAS J173454-1423.3 |
ASASSN-V J173454.32-142317.9 |
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GSC2.3 S811091161 |
NSVS 16598986 |
OGLE-BLG-LPV-242634 |
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OGLE-IV BLG813.29.4 |
UCAC4 379-085690 |
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| Variability type |
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M |
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| Spectral type |
-- |
| Mag. range |
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13.9 - <16.5 V |
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| Discoverer |
-- |
| Epoch |
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| Outburst |
-- |
| Period |
274.3: 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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J= 9.24; J-K= 1.60. ASAS-3 and NSVS magnitudes contaminated by UCAC4 379-085692 (V= 16.0; sep. 21"). NSVS magnitudes also contaminated by several other nearby stars. 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 |
Henden, A. A.; et al., 2016, AAVSO Photometric All Sky Survey (APASS) DR9 |
2016yCat.2336....0H |
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3 |
Wozniak, P. R.; et al., 2004, Northern Sky Variability Survey: Public Data
Release |
2004AJ....127.2436W |
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4 |
Pojmanski, G., 2002, The All Sky Automated Survey |
2002AcA....52..397P |
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5 |
CBAT "Transient Object Followup Reports" |
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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 = 9.24 | H = 8.32 | K = 7.64 | J - K = 1.59 |
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AllWISE
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W1 = 7.09 | W2 = 6.56 | W3 = 5.80 | W4 = 4.86 | W1 - W2 = 0.52 | W3 - W4 = 0.94 |
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APASS-DR9
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B = 16.05 | V = 14.26 | g' = 15.06 | r' = 13.48 | i' = 11.20 | B - V = 1.79 |
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Images
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Supporting Documents
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Revision History
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