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Latest Details
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Log in to retrieve additional aliases from SIMBAD. |
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| Name |
BMAM-V884 |
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| AAVSO UID |
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000-BPP-391 (No observations) |
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| Constellation |
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| J2000.0 |
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| B1950.0 |
07 56 32.58 +33 00 20.9 |
| Galactic coord. |
188.157 +27.836 |
Other names
(Internal only)
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1SWASP J075943.95+325206.9 |
2MASS J07594387+3252072 |
GSC 02472-00597 |
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TIC 361980195 |
TYC 2472-597-1 |
UCAC4 615-042983 |
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USNO-A2.0 1200-05901708 |
USNO-B1.0 1228-0204938 |
WISE J075943.88+325207.3 |
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| Variability type |
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EA |
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| Spectral type |
F2 |
| Mag. range |
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11.90 - 12.40 V |
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| Discoverer |
Mariusz Bajer |
| Epoch |
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| Outburst |
-- |
| Period |
17.34977 d |
| Rise/eclipse dur. |
1.5% (0.260 d) |
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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 |
Bajer, Mariusz
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Spectroscopic binary (2022ApJS..258...26Z). Highly eccentric system. Min II = 12.22 V at phase 0.802, duration 2.0%. BP-G= 0.27 (Gaia DR3); B-V= 0.56 (APASS); J-K= 0.16 (2MASS). ASAS-SN and SuperWasp magnitudes contaminated by Gaia DR3 881254755733303808 (V= 12.2; sep. 2.7"). Range has been corrected. The contamining star is the third body of the system, it is also a visual component (2020ApJS..246....4T). Parallax and proper motions from Gaia DR3 for BMAM-V884: Plx= 1.9833 +/- 0.0151 mas, PmRA= -8.860 +/- 0.014 mas/yr, PmDE= -12.699 +/- 0.012 mas/yr. Parallax and proper motions for Gaia DR3 881254755733303808: Plx= 2.0069 +/- 0.0144 mas, PmRA= -9.222 +/- 0.014 mas/yr, PmDE= -12.453 +/- 0.011 mas/yr. |
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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 |
Zhang, B.; et al., 2022, The Spectroscopic Binaries from the LAMOST
Medium-resolution Survey. I. Searching for Double-lined Spectroscopic
Binaries with a Convolutional Neural Network |
2022ApJS..258...26Z |
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Tian, H.-J.; et al., 2020, The Separation Distribution of Ultrawide
Binaries across Galactic Populations |
2020ApJS..246....4T |
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Xiang, M.; et al., 2019, Abundance Estimates for 16 Elements in 6 Million
Stars from LAMOST DR5 Low-Resolution Spectra |
2019ApJS..245...34X |
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Kochanek, C. S.; et al., 2017, The All-Sky Automated Survey for Supernovae
(ASAS-SN) Light Curve Server v1.0 |
2017PASP..129j4502K |
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Ricker, G. R.; et al., 2014, Transiting Exoplanet Survey Satellite (TESS) |
2014SPIE.9143E..20R |
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Butters, O. W.; et al., 2010, The first WASP public data release |
2010A&A...520L..10B |
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External Links
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Location
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Images
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Please review Digitized Sky Survey Acknowledgment and Copyright.
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Supporting Documents
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1 |
BMAM-V884 phase plot
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Bajer, Mariusz
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2023-04-04 17:22 UTC |
Phase plot data from ASAS-SN (V), ASAS-SN (g'), TESS SAP and SuperWASP (CV) shifted to V standard with zoom on primary and secondary eclipse. |
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Revision History
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