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Details for Revision 3
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Name
N Per 2020
AAVSO UID
000-BNS-429 (94628
observations
)
Constellation
Perseus
Sequence
J2000.0
04 29 18.85 +43 54 23.0 (67.32854 +43.90639)
Search nearby
B1950.0
04 25 46.09 +43 47 49.5
Galactic coord.
158.895 -3.234
Other names
(Internal only)
AT 2020abap
GSC2.3 NCFY024154
Gaia21awm
IPHAS J042918.86+435423.0
MASTER OT J042918.83+435423.7
Nova Per 2020
Nova Persei 2020
PGIR20fbf
PSO J042918.853+435423.044
TCP J04291884+4354232
TCP J04291888+4354233
USNO-A2.0 1275-03332809
USNO-B1.0 1339-0102783
ZTF20adaalge
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Variability type
N
Spectral type
--
Mag. range
8.6 - 20.1 V
Discoverer
Seiji Ueda
Epoch
--
Outburst
2020
Period
--
Rise/eclipse dur.
--
Remarks
Some references may be clicked to view in new window. Roll over index number to view submission details.
1
Schaefer, Brad
The 2.225 hour period published in CBET 4906 cannot be correct because (1) the periodicity produces a DFT peak that is lower than many other DFT peaks in the original data, so the period claim was insignificant, (2) the periodicity does not appear in the TESS light curve with amplitude limits of 0.000098 mag. (
2021RNAAS...5..150S
), nor in contemporaneous AAVSO data, and (3) novae before the transition phase, including around the peak, cannot display any coherent periodicity because the opaque shell hides the inner binary.
2
Schmeer, Patrick
The object shows a transition from a nova with some He/N spectral characteristics to a nova of the Fe II class, which is in the opposite sense of the transition observed in hybrid ("Fe IIb") novae (
2020ATel14230....1B
).
3
Schmeer, Patrick
Galactic classical Fe II nova (
2020ATel14229....1M
)
4
Schmeer, Patrick
Apparently independent discovery by Stanislav Korotkij, Kirill Sokolovskij, and Ol'ga Smol'yankina (CBAT "Transient Object Followup Reports"). No brightenings were recorded by the ASAS-SN Sky Patrol between 2014 December 16 and 2020 November 25.
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References
Click reference title/citation to view in new window. Roll over index number to view submission details.
1
Schaefer, B. E., 2021, Discovery of 13 New Orbital Periods for Classical
Novae
2021RNAAS...5..150S
2
Gaia Alerts, 2021 (online data)
--
3
R. E. Schmidt, 2021, CBET #4906
--
4
S. Borthakur; V. Kumar; V. Joshi; et al., 2020, ATel #14230
2020ATel14230....1B
5
U. Munari; P. Ochner; P. Valisa; S. Dallaporta, 2020, ATel #14229
2020ATel14229....1M
6
U. Munari; F. Castellani; S. Dallaporta; V. Andreoli, 2020, ATel #14224
2020ATel14224....1M
7
S. Nakano; S. Ueda; S. Korotkiy; et al., 2020, CBET #4890
--
8
CBAT "Transient Object Followup Reports", 2020 (online data)
--
9
J. Shears, 2020, vsnet-alert #25003
--
10
CBAT "Transient Object Followup Reports", 2020
--
11
Transient Name Server, 2020 (online data)
--
12
Kochanek, C. S.; et al., 2017, The All-Sky Automated Survey for Supernovae
(ASAS-SN) Light Curve Server v1.0
2017PASP..129j4502K
13
ZTF observations (Lasair online data)
--
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Supporting Documents
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Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
8
Schaefer, Brad
2021-07-13 15:00 UTC
Dubious period deleted.
7
Otero, Sebastian Alberto
2021-04-01 04:06 UTC
Gaia Alerts name and reference added.
6
Schmeer, Patrick
2021-01-11 08:24 UTC
Orbital period from CBET 4906. Type (NA) from AAVSO data. ZTF transient designation and reference added.
5
Otero, Sebastian Alberto
2021-01-04 22:50 UTC
Maximum magnitude and epoch of outburst peak from AAVSO data.
4
Schmeer, Patrick
2020-11-29 13:10 UTC
Primary name from CBET 4890. Maximum magnitude and epoch (optical peak) from AAVSO data.
3
Schmeer, Patrick
2020-11-28 02:29 UTC
Maximum magnitude from
2020ATel14229....1M
.
2
Schmeer, Patrick
2020-11-26 04:39 UTC
Type from
2020ATel14224....1M
. Primary name changed. Eruption year added. Maximum magnitude from AAVSO data. Minimum magnitude derived from Pan-STARRS1 and IPHAS DR2.
1
Otero, Sebastian Alberto
2020-11-26 03:45 UTC
Maximum magnitude from vsnet-alert 25003. Minimum magnitude from IPHAS DR2. Gaia DR2 position.
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