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Name
  NSV 18809  
AAVSO UID
000-BNV-133 (123 observations)  
Constellation
Centaurus Sequence
J2000.0
11 36 34.84 -61 36 35.2  (174.14517 -61.60978) Search nearby
B1950.0 11 34 14.33 -61 19 58.7
Proper motion
RA: -6.808 +/- 0.045 mas/yDec: 0.784 +/- 0.050 mas/ySource: Gaia DR1
Galactic coord. 294.157 -0.020
Other names

(Internal only)
ASAS J113635-6136.6 CD-60 3636 CPD-60 3161
HD 306799 HIP 56619 IRAS 11342-6120
NGC 3766 48 NGC 3766 MMU 48 NGC 3766 SHER R
PPM 358834 SAO 251483 TYC 8972-2273-1
[A72c] 63    
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Variability type
LC
Spectral type M0Ib
Mag. range
7.48 - 7.55 V
Discoverer --
Epoch
--
Outburst --
Period --
Rise/eclipse dur. --
Remarks
There are currently no remarks on file for this star. (Not logged in)  Add remark
References
Click reference title/citation to view in new window. Roll over index number to view submission details.
1 Pojmanski, G., 2002, The All Sky Automated Survey 2002AcA....52..397P
2 The Hipparcos and Tycho Catalogues, Vol.11 and Vol.17, CD-ROM No.1,
SP-1200, ESA, 1997.		 1997ESASP1200.....P
External Links
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Location    Go   
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Catalog Data
Information from selected catalogs obtained by cross-matching to 2 arc seconds using the CDS X-Match Service. These data may not be complete.
2MASS J = 4.56H = 3.46K = 3.20J - K = 1.36
AllWISE W2 = 2.95W3 = 2.92W4 = 2.80W3 - W4 = 0.12
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 11 36 34.84 -61 36 35.2 (J2000)
Source STScI
Survey

Red, all sky, 1.0 arcsec/pixel
  Negative
Supporting Documents
There are currently no supporting documents on file for this star. (Not logged in)  Add document
Stellar Association Membership
 NGC 3766 Open Cluster 2012A&A...548A..97Z
Campaigns/Programs
 SNEWS Campaign
Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
2 Otero, Sebastian Alberto 2021-01-20 20:44 UTC Type and range from Hipparcos, GCPD and ASAS-3 data. Gaia EDR3 position.
1 Admin, VSX 2005-12-18 01:33 UTC Preserved original object data.

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