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Query : Chi1 Orionis |
Basic data : | ||||||||||||||||||||||||||||||||||||||
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The link on the acronym of the identifiers give access to the
information for this acronym in the dictionary of nomenclature.
Identifiers (58) :
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* 54 Ori | GJ 222 | PPM 95062 | UBV 6000 |
* chi01 Ori | GSC 01320-02118 | 2RE J055423+201637 | USNO-B1.0 1102-00091548 |
** KNG 1 | HD 39587 | 2RE J0554+201 | USNO 815 |
AG+20 592 | HIC 27913 | RE J0554+201 | uvby98 100039587 |
ASCC 755242 | HIP 27913 | RE J055423+201609 | V* chi01 Ori |
BD+20 1162 | HR 2047 | ROT 942 | WDS J05544+2017AB |
CCDM J05544+2017AB | IRAS 05514+2016 | 1RXS J055423.4+201630 | WEB 5465 |
2E 1584 | IRC +20126 | SAO 77705 | WISE J055422.93+201634.9 |
2E 0551.4+2016 | JP11 1278 | SBC9 1535 | YZ 20 2042 |
2EUVE J0554+20.2 | LSPM J0554+2016 | SKY# 9763 | Zkh 78 |
EUVE J0554+20.2 | LTT 11743 | SPOCS 288 | Zkh 79 |
GAT 1261 | 2MASS J05542300+2016344 | TD1 5547 | Gaia DR2 3399063235753901952 |
GC 7419 | NLTT 15782 | TIC 114776214 | Gaia DR3 3399063235755057792 |
GCRV 3663 | PLX 1354 | TYC 1320-2118-1 | |
GEN# +1.00039587 | PLX 1354.00 | UBV M 11584 |
References (75 between 2019 and 2024) (Total 858)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). Follow new references on this object |
Warning : measurements from IRAS, IRC, SAO, CL.g (ACO), GJ have been removed
velocities (20)
|typ| Value R m.e. |A (Nmes)|na,Q,dom , res D| Obs.date | Rem. |Or| Reference | ------------------------------------------------------------------------------------------------------ |v | -15.5 | ( )|s , ,Opt , | | | |2023ApJS..266...41P|
v* (1)
| vartyp | Vmax p Vmin | period | epoch (JD) |D/rt %| reference | ----------------------------------------------------------------------------------------------------- |ROT | | 5 | | |1996ApJ...457L..99B|
diameter (1)
|diameterQ unit| error | filter | method | reference | --------------------------------------------------------------- |1.10E+00 mas |1.80E-02| |Interfer|2009ApJ...694.1085V|
distance (3)
| distance Q unit| err- err+ | method | reference | ----------------------------------------------------------------------- | 8.6994 pc | -0.0399 +0.0399 |paral |2020yCat.1350....0G|
rot (8)
| Vsini [ err ] (mes)|Q| reference | ------------------------------------------------- m| 10.79 [ ] ( )| |2010A&A...520A..79M|
fe_h (74)
| Teff log.g | Fe_H c|CompStar |CatNo| Reference | ------------------------------------------------------------ | 5913 4.34 |-0.10 |SUN | |2023ApJS..266...41P|
plx (5)
| plx : m.e R | reference | ------------------------------------------------ m| 115.43 : 1.08 |1997A&A...323L..49P|
pm (5)
| pm-ra [ m.e ]| pm-de [ m.e ]|syst| reference | -------------------------------------------------------------------- | -179.014[ 0.405]| -90.730[ 0.337]|ICRS|2020yCat.1350....0G|
mk (27)
|ds/mss| Spectral type | reference | ----------------------------------------------------------------- m| / |G0V |1989ApJS...71..245K|Observing logs
Warning : measurements from IRAS, IRC, SAO, CL.g (ACO), GJ have been removed
iue (76)
|Homogenized Name: ComplID |PROG |CL|D CAM IMAGE A| FES MD|Obs.da Time |ExpTim|m|CEB|S| Comments |F| reference | --------------------------------------------------------------------------------------------------------------------------------------- |HD 39587 : |STFTS|44|L SWP 22246 L| 383 FU|840211 202600|001800| |X32|G|E=61,C=1.1X,B=36 |*|1996IUEML.C......0I|
xmm (1)
B/xmm/xmmlog Post annotation | XMM-Newton Observation Log (XMM-Newton Science Operation Center, 2012) [ReadMe+ftp] 2002yCat....102009X The XMM-Newton Observation log (2024-07-01)[image/fits] (17783 rows) |
Full _r Obsno PropDate Object RAJ2000 DEJ2000 Obs0 ObsDur Image PPSp FITS XSAlink arcmin s deg deg s s
1 0.0002 0111500101 2002-09-28 Chi1 Orionis 088.59576 +20.27617 2001-04-07T08:56:49 48910 FITS PPSp 0111500101 Y
Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center
Data at NED - NASA/IPAC Extragalactic Database : Chi1 Orionis
Link by name to the catalogue in VizieR :
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