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Details for Revision 2
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Name
V0854 Cen
AAVSO UID
--
Constellation
Centaurus
Sequence
J2000.0
14 34 49.41 -39 33 19.2 (218.70587 -39.55533)
Search nearby
B1950.0
14 31 41.60 -39 20 12.8
Galactic coord.
323.769 +19.097
Other names
(Internal only)
Please note that aliases shown in grey link to obsolete records.
AAVSO 1428-39
ASAS J143450-3933.5
CD-39 9021
NSV 6708
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Variability type
RCB
Spectral type
--
Mag. range
6.84 - 14.94 V
Discoverer
--
Epoch
--
Outburst
--
Period
--
Rise/eclipse dur.
--
Remarks
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1
Otero, Sebastian Alberto
Pulsation period: 43.23 days.
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References
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1
2002AcA....52..397P
Pojmanski, G., 2002, Acta Astronomica, 52, 397, The All Sky Automated
Survey
2
1999AJ....117.3007L
Lawson, W.A., Maldoni, M.M., Clayton, G.C., Valencic, L., Jones, A.F.,
Kilkenny, D., van Wyk, F., Roberts, G., Marang, F., 1999, The Astronomical
Journal, Volume 117, Issue 6, pp. 3007-3020
3
Tisserand, P.; Clayton, G. C.; Bessell, M. S.; et al., 2020, A plethora of
new R Coronae Borealis stars discovered from a dedicated spectroscopic
follow-up survey
2020A&A...635A..14T
4
Gaia Collaboration; et al., 2018, Gaia Data Release 2. Summary of the
contents and survey properties
2018A&A...616A...1G
5
J. Alfonso-Garzon, A. Domingo, J.M. Mas-Hesse, A. Gimenez, 2012,
arXiv:1210.0821 [astro-ph.IM] (online info)
2012arXiv1210.0821A
6
G.Pojmanski, Acta Astronomica 52, 397, 2002.
2002AcA....52..397P
7
M.Feast, IAU Circ No.4651,1988.
1988IAUC.4651....0F
8
R.H.McNaught, G.Dawes, IBVS N2928,1986.
1986IBVS.2928....1M
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Supporting Documents
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1
Historical light curve
Otero, Sebastian Alberto
2011-04-25 01:27 UTC
Observations from the literature and the AAVSO database.
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Campaigns/Programs
Binocular program
Individual campaigns
Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
5
Otero, Sebastian Alberto
2020-06-10 02:48 UTC
Reference to
2020A&A...635A..14T
added. Gaia DR2 position.
4
Otero, Sebastian Alberto
2020-05-15 00:03 UTC
Gaia DR2 position.
3
Otero, Sebastian Alberto
2011-04-25 01:27 UTC
Updated minimum magnitude from Di Scala CCDV-data. Spectral type from Skiff (2010).
2
Otero, Sebastian Alberto
2006-07-26 18:24 UTC
V observatons from the literature and the ASAS-3 database show a larger amplitude
1
Admin, VSX
2005-12-18 01:33 UTC
Initial database population.
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