|
|
Revise New Search
|
Details for Revision 1
|

|
Log in to retrieve additional aliases from SIMBAD. |
|
Name |
V2553 Sgr |
|
|
AAVSO UID |
000-BFG-907 (No observations) |
|
|
Constellation |
|
J2000.0 |
|
B1950.0 |
18 24 32.41 -23 17 54.7 |
Galactic coord. |
9.548 -5.460 |
Other names

(Internal only)
|
2MASS J18273473-2316005 |
ASAS J182735-2316.0 |
|
(Not logged in) Add name
|
Variability type |
M |
|
|
Spectral type |
M: |
Mag. range |
14.4 - <16.0 p |
|
|
Discoverer |
-- |
Epoch |
|
Outburst |
-- |
Period |
193 d |
Rise/eclipse dur. |
-- |
|
|
Remarks
|

|
Some references may be clicked to view in new window. Roll over index number to view submission details.
|
|
1 |
Otero, Sebastian Alberto
|
VSP Note: 15.3 mag. star 5" to the SSE and 15.3 mag. star 13" to the W. |
2 |
Otero, Sebastian Alberto
|
Crowded area. ASAS-3 magnitudes contaminated by 2MASS J18273482-2316052 (= NSV 10819; V= 15.3; sep. 5"), 2MASS J18273543-2315519 (V= 17.4; sep. 13"), 2MASS J18273377-2315596 (V= 15.3; sep. 13"), 2MASS J18273530-2315474 (V= 16.7; sep. 15"), 2MASS J18273479-2316166 (V= 16.9; sep. 16") and 2MASS J18273341-2316004 (V= 16.4; sep. 18"). Range has been corrected. |
|
|
(Not logged in) Add remark
|
|
References
|

|
Click reference title/citation to view in new window. Roll over index number to view submission details.
|
|
1 |
Iwanek, P.; et al., 2022, The OGLE Collection of Variable Stars: Nearly 66,000 Mira Stars in the Milky Way |
2022ApJS..260...46I |
2 |
Pojmanski, G., 2002, The All Sky Automated Survey |
2002AcA....52..397P |
3 |
D.Hoffleit, IBVS N660, 1972. |
1972IBVS..660....1H |
4 |
D.Hoffleit, AJ 72, 711, 1967. |
1967AJ.....72..711H |
|
|
|
External Links
|

|
Links open in a new window. Not all links may be valid for this particular target.
|
|
Location
|
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.
|
|
|