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Details for Revision 2
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Log in to retrieve additional aliases from SIMBAD. |
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Name |
FQ Cir |
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AAVSO UID |
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Constellation |
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J2000.0 |
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B1950.0 |
15 20 40.99 -60 49 12.3 |
Galactic coord. |
320.469 -3.459 |
Other names

(Internal only)
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2MASS J15244761-6059472 |
ASAS J152447-6059.8 |
ASASSN-22ii |
AT 2022nyt |
CWISE J152447.57-605947.6 |
DENIS J152447.6-605947 |
GALEX J152447.5-605947 |
GSC2.3 S7QD034895 |
Gaia22cse |
SMSS J152447.58-605947.5 |
TCP J15244460-6059200 |
UCAC2 05164744 |
UCAC4 146-178435 |
USNO-A2.0 0225-22585493 |
USNO-B1.0 0290-0615824 |
WISE J152447.54-605947.8 |
WISEA J152447.58-605947.7 |
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(Not logged in) Add name
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Variability type |
N: |
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Spectral type |
-- |
Mag. range |
10.9 - 14.1 g |
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Discoverer |
Andrew Pearce |
Epoch |
25 Jun 2022 (HJD 2459755.7) |
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Outburst |
2022 |
Period |
-- |
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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First published as variable in 2021MNRAS.503.3975P. Increased activity between 2019 and 2021. |
2 |
Schmeer, Patrick
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"The low amplitude of the transient raises questions about its nature and the possible progenitor match. There is a slight chance that the actual progenitor system is much fainter and coincides with the bright (~14 mag) match" (2022ATel15473....1A). 0.1-0.2 mag. variations in historical ASAS-SN data. Gaia DR3 parallax (for Gaia DR3 5875610751015084544): 0.11 ± 0.02 mas (distance 6.5 ± 0.8 kpc). Derived Mv ∼-1 is too bright for a nova. |
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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 |
Creevey, O. L.; et al., 2023, Gaia Data Release 3: Astrophysical parameters inference system (Apsis) I -- methods and content overview |
2023A&A...674A..26C |
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E. Aydi; K. V. Sokolovsky; J. Strader; et al., 2022, ATel #15473 |
2022ATel15473....1A |
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A. Pearce; F. Romanov; R. H. McNaught; et al., 2022, CBET No. 5135 |
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CBAT "Transient Object Followup Reports", 2022 (online data) |
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Petrosky, E.; et al., 2021, Variability, periodicity, and contact binaries in WISE |
2021MNRAS.503.3975P |
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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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External Links
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Location
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Supporting Documents
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There are currently no supporting documents on file for this star.
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Revision History
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Currently approved revision is checked. Click revision number to view details of that revision.
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