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IPs

AE Aqr
FO Aqr
XY Ari
V405 Aur
HT Cam
MU Cam
DW Cnc
BG CMi
V709 Cas
V1025 Cen
TV Col
TX Col
UU Col
V2306 Cyg
YY Dra
PQ Gem
DQ Her
EX Hya
NY Lup
V2400 Oph
GK Per
AO Psc
WX Pyx
V1223 Sgr
V1062 Tau
RX J2133

Related Systems

Candidates

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The Curmudgeon's List of IP Candidates


This is so far a partial list of IP candidates. The Curmudgeon will be adding his comments on
V533 Her, HZ Pup, V795 Her, V426 Oph, and TW Pic in the near future.

Here is a list of objects that will not be included: V603 Aql, V1432 Aql, TT Ari, AH Eri, VZ Pyx, SW UMa, KO Vel, and V407 Vul.


CandidatePeriodsThe Curmudgeon's Verdict
V1425 Aql =
Nova Aquilae 1995
Porb=6.139hr
Pspin=86.5min?
Pbeat=1.89hr??
Pro: The detection of three periods is based on extensive photometry.
Con: The system was still well above pre-nova brightness at the time of these observations.
Verdict: A solid candidate on paper, yet the Curmudgeon is uneasy. An independent confirmation, with the system closer to pre-nova brightness, would convince him.
RR Cha =
Nova Chamaeleontis 1953
Porb=3.362hr
Pspin=32.5min?
Pro: The orbital period of 3.362 hr is beyond doubt from the eclipses; 1950s photometric period is claimed from Feb 2001 and May 2001 photometry runs.
Con: Are they (particularly Feb 2001 detection) definitely above the general red noise?
Verdict: The Curmudgeon is not convinced.
DD Cir =
Nova Circinus 1999
Porb=2.339hr
Pspin=670s?
Pro: The orbital period of 2.339 hr is beyond doubt from the eclipses.
Con: The ~670 s signal was not seen in all of their photometry runs.
Verdict: The Curmudgeon is not convinced.
AP Cru =
Nova Curcis 1935
Porb=5.12hr(?)
Pspin=1837s?
Pro: None.
Con: Even the credentials as CV is still up for debate. The claimed 1837 s signal is transient.
Verdict: The Curmudgeon would be surprised.
WZ Sge Porb=1.3605hr
Pspin=27.87s?
P???=28.96s
Pro: ASCA data appears to have the 27.87 s period. Bill Welsh can't make the pulsation model work.
Con: If there is a signal in the XMM-Newton data, it's the 28.96 s one. Joe Patterson can't make the numerology work in the IP model.
Verdict: The Curmudgeon is confused.
V697 Sco =
Nova Sorpii 1941
Porb=4.49hr
Pspin=3.31hr?
Pro: Multiple peaks are seen in the FT.
Con: Too many peaks are seen in the FT. An IP interpretation emerges if and only if it is assumed that these are due to strictly periodic clocks.
Verdict: The Curmudgeon only sees quasiperiodic variability in V697 Sco.
V373 Sct =
Nova Scuti 1975
Porb=???
Pspin=258.3s?
Pro: One of three photometry runs shows a signal at 258.3 s.
Con: The other two don't.
Verdict: The Curmudgeon is skeptical.
V381 Vel =
RXJ1016.9-4103
Porb=134min?
Pspin=122min?
Pro: 122 and 134 min periods seen.
Con: Greiner & Schwarz, who prefer 134 min, say "common periods of 123, 134, and 149 min are possible" due to poor sampling.
Verdict: Evidence for the 134 min period is weak. An umbiguous detection of it in better sampled data is necessary to convine The Curmudgeon
Aqr 1 =
2236+0052 =
SDSSJ223843.84+010820.7
Porb=122min?
Pspin=6.728min?
Pro: Detection of the 6.723 min period is convincing
Con: The orbital period is uncertain and the possible sideband features don't match up neatly with the reported orbital period.
Verdict: A good candidate. An independent confirmation would be nice.
HS0922+1333 Porb=4.6hr?
Pspin=4.1hr?
Pro: Photometric and spectroscopic periods differ
Con: Both observations barely cover one cycle
Verdict: Not convincing. The Curmudgeon will reconsider if longer observations confirm the dual periodicity.
1RXS J015317.9+744641 Porb=3.94 hr
Pspin=1974 s?
Pro: Spin-like modulations seen in X-rays and in the optical.
Con: Orbital period is cited in catalogs via private communication, with no actual publication. Recent optical photometry only covers 7 or so beat cycles.
Verdict: This one looks like a genuine IP, but more data are required before The Curmudgeon will list this among the confirmed.
VZ Sex = RX J0944.5+0357 Porb=3.581hr
Pspin=2162s?
Pro: Spectroscopy establishes the 3.581 hr orbital period; the 2162 s period is clearly visible in some light curves.
Con: ...but not in others (Mennickent et al. did not see this period). Aperiodic variability is strong.
Verdict: It will take a repeated appearances of this period to convince The Curmudgeon.
YY Sex = RX J1039.7-0507 Porb=1.574hr
Pspin=1443.7s?
Pro: Strong orbital photometric modulation (reflection) and additional power seen.
Con: Are the FT peaks all due to real and strictly periodic signals, given the general red noise pluse the possible presence of higher harmonics of the orbital period?
Verdict: The Curmudgeon is not convinced, and will wait for the results of the XMM-Newton observation.
Swift J0732.5-1331 Porb=5.604 hr
Pspin=512.42s
Pro: All observations reported so far are consistent with IP interpretation.
Con: We only have ATels so far, possibly from relatively sparse data.
Verdict: The Curmudgeon is waiting for refereed publications to make it official.

(Page last updated 2006 April 17)


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    This file was last modified on Monday, 14-Aug-2006 10:54:39 EDT