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Name
T CrB
AAVSO UID
Constellation
J2000.0
B1950.0
15 57 24.58 +26 03 40.0
Galactic coord.
42.374 +48.165
Other names(Internal only)
Please note that aliases shown in grey link to obsolete records.
1SXPS J155930.1+255514
3XMM J155930.1+255512
AAVSO 1555+26
ASAS J155930+2555.2
ASASSN-V J155930.27+255511.9
BD+26 2765
HD 143454
HIP 78322
HR 5958
MWC 413
N CrB 1866
Nova Coronae Borealis 1866
Nova CrB 1866
SAO 84129
SWIFT J1559.6+2554
X 15574+261
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Variability type
NR
Spectral type
M3III+pec(NOVA)
Mag. range
2 - 10.8 V
Discoverer
--
Epoch
Outburst
1946
Period
(29000 d) (79.40 y)
Rise/eclipse dur.
--
Remarks
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1
Schmeer, Patrick
Discovered on 1866 May 12 by John Birmingham. First nova to be identified with an existing star (BD +26°2765, 9.5 mag). Second known eruption detected independently by Norman F. H. Knight (1946 Feb. 9.25 UT) and Armin Joseph Deutsch (Feb. 9.35 UT). Gaia DR2 parallax 1.2127 ± 0.0488 mas (distance 806 ± 33 pc).
2
Otero, Sebastian Alberto
Amplitude for ELL variations 0.45 mag. GCVS outburst cycle 29,000 days.
3
GCVS Team
VB? A (B <= 12m, 0.2"). SB (P = 227.6d). The spectral period is present in the photometric data of 1891 - 1917 and 1960 - 1971 [J.Bailey, JBAA 85, N3, 217, 1975. ]. The epoch of the first outburst JD2402734 (1866). Two smaller outbursts were observed in UV light, JD2438030 (1963) and 2442543 (1975) [L.H.Palmer, J.L.Africano, IBVS N2069, 1982. ].
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References
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1
Maslennikova, N. A.; Tatarnikov, A. M.; Tatarnikova, A. A.; et al., 2023,
2023arXiv230810011M
2
M. Gromadzki, J. Mikolajewska, I. Soszynski, 2013, arXiv:1312.6063
2013arXiv1312.6063G
3
R.A. Downes et al., 2001, PASP 113, 764 (2006 archival version)
2005JAD....11....2D
4
G.Pojmanski, Acta Astronomica 52, 397, 2002.
2002AcA....52..397P
5
R.A. Downes et al., 2001, PASP 113, 764
2001PASP..113..764D
6
Herbig, G. H.; Neubauer, F. J., 1946, The Spectrum of T Coronae Borealis at
1946PASP...58..196H
7
Birmingham, J., 1866, The new variable near η Coronae
*** Please covert MNRAS 26 (1866), 310 to bibcode ***
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Campaigns/Programs
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Revision History
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