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Query : Hip 46517 |
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Hierarchy :
number of linked objects
whatever the membership probability is (see description here ) :
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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 (25) :
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HD 82165
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GSC 07691-00764
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SKY# 18324 | WEB 8780 |
CD-37 5817
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HIC 46517
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TD1 13985
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Gaia DR2 5429897771019708672
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CPC 18 4322 |
HIP 46517
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TIC 5165416 |
Gaia DR3 5429897771019708672
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CPD-37 3549
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HR 3766
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TYC 7691-764-1
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Gaia DR1 5429897766720761856
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GC 13094 |
2MASS J09291618-3824127
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UBV 9062 | |
GCRV 60681 |
PPM 286516
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UBV M 15455 | |
GEN# +1.00082165 |
SAO 200419
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uvby98 100082165
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References (5 between 2019 and 2024) (Total 30)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). ![]() |
Warning : measurements from IRAS, IRC, SAO, CL.g (ACO), GJ have been removed
velocities (4)
|typ| Value R m.e. |A (Nmes)|na,Q,dom , res D| Obs.date | Rem. |Or| Reference | ------------------------------------------------------------------------------------------------------ |v | 0.6 | ( 4)|s , , , | | | |1995A&AS..114..269D|
distance (2)
| distance Q unit| err- err+ | method | reference | ----------------------------------------------------------------------- | 60.890 pc | -0.0823 +0.0823 |paral |2020yCat.1350....0G|
fe_h (1)
| Teff log.g | Fe_H c|CompStar |CatNo| Reference | ------------------------------------------------------------ | 7492 | | | |2006A&A...450..735M|
plx (5)
| plx : m.e R | reference | ------------------------------------------------ | 16.423 : 0.0222 |2020yCat.1350....0G|
pm (5)
| pm-ra [ m.e ]| pm-de [ m.e ]|syst| reference | -------------------------------------------------------------------- | -106.194[ 0.018]| +3.009[ 0.021]|ICRS|2020yCat.1350....0G|
mk (3)
|ds/mss| Spectral type | reference | ----------------------------------------------------------------- | / |A2 |1993yCat.3135....0C|
Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center
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