AAVSO Home



Welcome, Guest. You are not logged in.
Log in
    Revise    New Search
Latest Details
Log in to retrieve additional aliases from SIMBAD.
Name
  V0607 Lyr  
AAVSO UID
000-BFR-450 (4 observations)  
Constellation
Lyra Sequence
J2000.0
19 20 49.19 +37 49 14.3  (290.20496 +37.82064) Search nearby
B1950.0 19 19 04.12 +37 43 31.9
Proper motion
RA: 1.6 +/- 7.2 mas/yDec: -3.4 +/- 5.6 mas/ySource: UCAC4
Galactic coord. 69.998 +10.937
Other names

(Internal only)
ASASSN-V J192049.19+374914.3 SBG 6777 (NGC 6791) V97 (NGC 6791)
(Not logged in)  Add name
Variability type
SRS:
Spectral type --
Mag. range
16.49 (0.08) V
Discoverer --
Epoch
--
Outburst --
Period 9.563 d
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 Bruntt, H., Grundahl, F., Tingley, B., et al. 2003, AsAp, 410, No. 1, 323. 2003A&A...410..323B
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.
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 = 14.45H = 13.93K = 13.80J - K = 0.65
AllWISE W1 = 13.72W2 = 14.02W1 - W2 = -0.30
Images
Please review Digitized Sky Survey Acknowledgment and Copyright.
Size 5' x 5' (297 x 298 pixels)
Center 19 20 49.19 +37 49 14.3 (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 6791 Open Cluster 2012A&A...548A..97Z
Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
2 Admin, VSX 2010-01-05 04:43 UTC Position updated from the GCVS version of November 2009.
1 Admin, VSX 2006-08-20 03:12 UTC Initial upload.