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Latest Details
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Log in to retrieve additional aliases from SIMBAD. |
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| Name |
HP Nor |
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| AAVSO UID |
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| Constellation |
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| J2000.0 |
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| B1950.0 |
16 16 50.15 -54 46 14.0 |
| Proper motion |
| RA: -7.2 +/- 4.0 mas/y | Dec: -11.2 +/- 4.0 mas/y | Source: UCAC4 |
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| Galactic coord. |
330.074 -3.458 |
Other names
(Internal only)
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Please note that aliases shown in grey link to obsolete records.
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AAVSO 1612-54 |
AN 773.1935 |
ASASSN-V J162049.54-545323.2 |
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Downes HP Nor |
GDS_J1620495-545323 |
HV 8865 |
(Not logged in) Add name
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| Variability type |
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UG |
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| Spectral type |
pec(UG) |
| Mag. range |
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12.8 - 16.41 V |
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| Discoverer |
-- |
| Epoch |
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| Outburst |
-- |
| Period |
(17.3 d) |
| Rise/eclipse dur. |
-- |
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Remarks
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There are currently no remarks on file for this star.
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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 |
R.A. Downes et al., 2001, PASP 113, 764 (2006 archival version) |
2005JAD....11....2D |
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2 |
R.A. Downes et al., 2001, PASP 113, 764 |
2001PASP..113..764D |
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3 |
N.Vogt, F.M.Bateson, AsAp Suppl 48, N3, 383, 1982. |
1982A&AS...48..383V |
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4 |
M.Petit, JO 43, 17, 1960. |
1960JO.....43...17P |
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5 |
AAVSO Light Curve |
-- |
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External Links
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Location
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Select a Location for more details.
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Catalog Data
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Information from selected catalogs obtained by cross-matching to 2 arc seconds using the CDS X-Match Service. These data may not be complete.
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2MASS
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J = 14.09 | H = 13.55 | K = 13.33 | J - K = 0.76 |
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AllWISE
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W1 = 12.59 | W2 = 12.55 | W1 - W2 = 0.04 |
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Images
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Please review Digitized Sky Survey Acknowledgment and Copyright.
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Image not downloaded. Click Retrieve Image to download and view. |
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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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Stellar Association Membership
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Harvard 10 |
Open Cluster |
2012A&A...548A..97Z |
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Campaigns/Programs
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Legacy CVs
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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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3 |
Linnolt, Mike
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2015-03-21 01:31 UTC |
Lightcurve when including "fainter than" observations precludes occurence of standstills during the pre-1997 period, which was previously used as evidence of standstill behavior using only positive observations. There remains little ,if any, significant evidence of this star being a UGZ subtype. |
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2 |
Admin, VSX
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2010-01-05 04:43 UTC |
Position updated from the GCVS version of November 2009. |
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1 |
Admin, VSX
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2005-12-18 01:33 UTC |
Initial upload. |
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