AAVSO Home
The International
Variable Star Index
Search
Submit
Register
Log In
Account
About
Welcome, Guest. You are not logged in.
Log in
Revise
New Search
Details for Revision 1
Log in to retrieve additional aliases from SIMBAD.
Name
V1223 Sgr
AAVSO UID
000-BCX-045 (207742
observations
)
Constellation
Sagittarius
Sequence
J2000.0
18 55 02.30 -31 09 50.0 (283.75958 -31.16389)
Search nearby
B1950.0
18 51 49.21 -31 13 41.5
Galactic coord.
4.958 -14.355
Other names
(Internal only)
Please note that aliases shown in grey link to obsolete records.
1RXP J18551.9-310946
1RXS J185502.1-310951
1WGA J1855.0-3109
2MASS J18550231-3109495
2RXP J185502.3-310954
2RXS J185502.1-310951
2XMM J185502.3-310948
3A 1851-312
3XMM J185502.2-310950
4U 1849-31
AAVSO 1848-31
ASASSN-V J185502.22-310950.9
Downes V1223 Sgr
UCAC4 295-217956
X 18518-312
XMMOM J185502.3-310949
XMMSL1 J185502.6-310937
XMMSL2 J185502.6-310939
(Not logged in)
Add name
Variability type
XPR
Spectral type
pec(e+cont)
Mag. range
13.26 - <16.3 B
Discoverer
--
Epoch
--
Outburst
--
Period
--
Rise/eclipse dur.
--
Remarks
Some references may be clicked to view in new window. Roll over index number to view submission details.
1
2009arXiv0910.0954S
White dwarf spin period = 746 seconds.
2
GCVS Team
As a rule has a persistent high state; five drops by two to more than three magnitudes have been registered and a twelve year interval of irregular variations at intermediate magnitudes. According to [
B.Warner, M.Cropper, MN 206, N2, 261, 1984.
] there are slow variations in brightness by 0.15m on a time scale of ~1 day. They are superimposed by variations with the orbital period P orb (Max = 2444749.9866 + 0.140239d*E) and with amplitude up to 0.15m. These variations in their turn are superimposed by the others: with P = 794.38s and the amplitude from 0.03m up to 0.15m (Max = 2444750.00404 + 0.009194215d*E and (sometimes) with P = 849.8s and a twice smaller amplitude (Max = 2444750.00350 + 0.00983588d*E). Besides there are rapid brightness variations on time scales 10 - 100s by 0.10m - 0.20m, and high frequency flickering by 0.05m. According to [
W.R.Penning, ApJ 289, 300, 1985.
], the period of X-ray pulses associated with the rotation of the compact object is 12.5 minutes.
(Not logged in)
Add remark
References
Click reference title/citation to view in new window. Roll over index number to view submission details.
1
T. Kato, 2020, vsnet-chat #8489
--
2
S. Scaringi et al., 2009, arXiv:0910.0954v1 [astro-ph.GA]
2009arXiv0910.0954S
3
R.A. Downes et al., 2001, PASP 113, 764 (2006 archival version)
2005JAD....11....2D
4
R.A. Downes et al., 2001, PASP 113, 764
2001PASP..113..764D
5
Garnavich, P.; Szkody, P., 1988, Observed Low States in DQ Herculis Systems
1988PASP..100.1522G
6
E.P.Belseren, BAAS 13, N2, 524, 1981.
1981BAAS...13Q.524B
7
J.E.Steiner, D.A.Schwartz, F.J. Jablonski, I.C.Busko, M.G.Watson, J.P.Pye,
I.M.McHardy, ApJ 249, L 21, 1981.
1981ApJ...249L..21S
External Links
Links open in a new window. Not all links may be valid for this particular target.
Location
-- Select --
AAVSO Variable Star Plotter
AAVSO Light Curve
AAVSO WebObs
APASS
AAVSOnet EPD
SIMBAD
SIMBAD Clickable Map
SIMBAD Coordinate query
VizieR Search
Aladin Java Applet
CDS Portal
CDS Biblio
SDSS Navigate Tool
GCVS
Downes
ASAS-SN Variable
ASAS-SN Sky Patrol
ASAS Light Curve
NSVS
CRTS
SuperWASP
Kamogata Wide-field Survey (KWS)
Go
Select a
Location
for more details.
Supporting Documents
There are currently no supporting documents on file for this star.
(Not logged in)
Add document
Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
6
Otero, Sebastian Alberto
2020-07-24 04:19 UTC
Type and minimum magnitude from
1988PASP..100.1522G
.
5
Otero, Sebastian Alberto
2020-07-13 23:00 UTC
Type and range from AAVSO data. Gaia DR2 position.
4
Otero, Sebastian Alberto
2011-05-18 01:45 UTC
Primary record creation. Type and range from Downes (2001).
3
Admin, VSX
2010-01-05 04:43 UTC
Position updated from the GCVS version of November 2009.
2
Admin, VSX
2009-10-09 02:29 UTC
Orbital period from [
2009arXiv0910.0954S
].
1
Admin, VSX
2005-12-18 01:33 UTC
Initial upload.
Guidelines
FAQ
Manual
Forum
Variability Types
Passbands
Copyright
Acknowledgments
Privacy
Contact
Help us
The International Variable Star Index
© 2005-2025 American Association of Variable Star Observers (AAVSO)
Version 1.1 [C]
172.30.0.162