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{{Starbox observe |
{{Starbox observe |
epoch=J2000 |
epoch=J2000 |
ra={{RA|14|49|41.29265}}<ref name="vanLeeuwen2007"/> |
ra=14<sup>h</sup> 49<sup>m</sup> 41.2935<sup>s</sup> |
dec= +48° 43&prime; 14.894&Prime; |
dec= {{DEC|+48|43|14.9077}}<ref name="vanLeeuwen2007"/> |
appmag_v=5.69 |
appmag_v=5.69<ref name=Priv/> |
constell=[[Boötes (constellation)|Boötes]] }}
constell=[[Boötes (constellation)|Boötes]] }}
{{Starbox character |
{{Starbox character |
class=F8V+F7V <ref name="abt"/>|
class=F8V+F7V<ref name="abt"/>|
r-i = |
r-i = |
v-r = |
v-r = |
b-v = +0.475<ref name=Priv>{{cite journal|title=Results of BV photometry 1969-70 (Uppsala refractor)|author1=Haggkvist, L.|author2=Oja, T.|journal=Private Communication|publisher=SIMBAD|bibcode=1970Priv.........0H}}</ref> |
b-v = 0.47 |
u-b = |
u-b = |
variable= }}
variable= }}
{{Starbox astrometry |
{{Starbox astrometry |
radial_v=&minus;30.90 ± 0.3<ref name=RV>{{cite journal|url=http://adsabs.harvard.edu/abs/2006AstL...32..759G|title=Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system|author=Gontcharov, G. A.|date=2006|journal=Astronomy Letters|volume=32|issue=11|pages=759–771|bibcode=2006AstL...32..759G|doi=10.1134/S1063773706110065|arxiv=1606.08053|accessdate=12 December 2016}}</ref> |
radial_v=-29.5 |
prop_mo_ra=-76.93 |
prop_mo_ra=&minus;77.94<ref name="vanLeeuwen2007"/> |
prop_mo_dec=99.13 |
prop_mo_dec= 100.83<ref name="vanLeeuwen2007"/> |
parallax=14.58|
parallax=14.58 |
p_error=0.51|
p_error=0.51 |
parallax_footnote =<ref name="vanLeeuwen2007"/> |
parallax_footnote =<ref name="vanLeeuwen2007"/> |
absmag_v=2.53<ref name=aaa361_614/> }}
absmag_v=2.53<ref name=aaa361_614/> }}
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Simbad=HD+131041
Simbad=HD+131041
| ARICNS = }}
| ARICNS = }}
{{starbox sources|HIP|CCDM|HR}}
{{Starbox reference |
Simbad=ADS+9406 }}
{{Starbox end}}
{{Starbox end}}


'''39 Boötis''' (abbr.: '''39 Boo''') or '''ADS 9406 B''' is a [[star]] in the [[constellation]] [[Boötes]]. A multiple star system, it has a combined [[apparent magnitude]] of 5.68. The system is 224 ± 8 light-years distant.
'''39 Boötis''' (abbreviated as '''39 Boo''') or '''ADS 9406 B''' is a [[star]] in the [[constellation]] [[Boötes]]. A multiple star system, it has a combined [[apparent magnitude]] of 5.68. The system is 224 ± 8 light-years distant.
<ref name="vanLeeuwen2007"/> It is composed of BD+49 2326A, which has an apparent magnitude of 6.248 and spectral type F8V, and BD+49 2326B, which has an apparent magnitude of 6.62 and spectral type F7V. Both stars are themselves spectroscopic binaries.<ref name="abt">{{cite journal|last=Abt, Helmut A.|date=2009|title=MK Classifications of Spectroscopic Binaries|journal=The Astrophysical Journal Supplement|volume=180|issue=1|pages=117–18|doi=10.1088/0067-0049/180/1/117 |bibcode=2009ApJS..180..117A}}</ref>
<ref name="vanLeeuwen2007"/> It is composed of BD+49 2326A, which has an apparent magnitude of 6.248 and spectral type F8V, and BD+49 2326B, which has an apparent magnitude of 6.62 and spectral type F7V. Both stars are themselves spectroscopic binaries.<ref name="abt">{{cite journal|last=Abt, Helmut A.|date=2009|title=MK Classifications of Spectroscopic Binaries|journal=The Astrophysical Journal Supplement|volume=180|issue=1|pages=117–18|doi=10.1088/0067-0049/180/1/117 |bibcode=2009ApJS..180..117A}}</ref>



Revision as of 23:28, 11 March 2017

39 Boötis
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes
Right ascension 14h 49m 41.29265s[1]
Declination +48° 43′ 14.9077″[1]
Apparent magnitude (V) 5.69[2]
Characteristics
Spectral type F8V+F7V[3]
B−V color index +0.475[2]
Astrometry
Radial velocity (Rv)−30.90 ± 0.3[4] km/s
Proper motion (μ) RA: −77.94[1] mas/yr
Dec.: 100.83[1] mas/yr
Parallax (π)14.58 ± 0.51 mas[1]
Distance224 ± 8 ly
(69 ± 2 pc)
Absolute magnitude (MV)2.53[5]
Details
Mass1.43[5] M
Rotational velocity (v sin i)161.0[5] km/s
Other designations
CCDM J14497+4843, HIP 72524, HR 5538, WDS J14497+4843, AG+48° 1158, HD 131041, SAO 45231, BD+49° 2326.
Database references
SIMBADdata

39 Boötis (abbreviated as 39 Boo) or ADS 9406 B is a star in the constellation Boötes. A multiple star system, it has a combined apparent magnitude of 5.68. The system is 224 ± 8 light-years distant. [1] It is composed of BD+49 2326A, which has an apparent magnitude of 6.248 and spectral type F8V, and BD+49 2326B, which has an apparent magnitude of 6.62 and spectral type F7V. Both stars are themselves spectroscopic binaries.[3]

References

  1. ^ a b c d e f van Leeuwen, F. (2007). "Validation of the New Hipparcos Reduction". Astronomy and Astrophysics. 474 (2): 653–64. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
  2. ^ a b Haggkvist, L.; Oja, T. "Results of BV photometry 1969-70 (Uppsala refractor)". Private Communication. SIMBAD. Bibcode:1970Priv.........0H.
  3. ^ a b Abt, Helmut A. (2009). "MK Classifications of Spectroscopic Binaries". The Astrophysical Journal Supplement. 180 (1): 117–18. Bibcode:2009ApJS..180..117A. doi:10.1088/0067-0049/180/1/117.
  4. ^ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. Retrieved 12 December 2016.
  5. ^ a b c Pizzolato, N.; Maggio, A.; Sciortino, S. (September 2000), "Evolution of X-ray activity of 1-3 Msun late-type stars in early post-main-sequence phases", Astronomy and Astrophysics, 361: 614–628, Bibcode:2000A&A...361..614P

Components

NAME Right ascension Declination Apparent magnitude (V) Spectral type Database references
ADS 9406 A (BD+49 2326A) 14h 49m 41.5s +48° 43' 09 6.2 F5 Simbad
ADS 9406 C (CCDM J14497+4843B) 14h 49m 41.8s +48° 43' 11 6.7 F5 Simbad