39 Boötis: Difference between revisions
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{{Starbox observe | |
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epoch=J2000 | |
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ra={{RA|14|49|41.29265}}<ref name="vanLeeuwen2007"/> | |
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ra=14<sup>h</sup> 49<sup>m</sup> 41.2935<sup>s</sup> | |
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dec= +48 |
dec= {{DEC|+48|43|14.9077}}<ref name="vanLeeuwen2007"/> | |
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appmag_v=5.69 | |
appmag_v=5.69<ref name=Priv/> | |
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constell=[[Boötes (constellation)|Boötes]] }} |
constell=[[Boötes (constellation)|Boötes]] }} |
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class=F8V+F7V |
class=F8V+F7V<ref name="abt"/>| |
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r-i = | |
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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> | |
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b-v = 0.47 | |
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variable= }} |
variable= }} |
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{{Starbox astrometry | |
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radial_v=−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> | |
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radial_v=-29.5 | |
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prop_mo_ra= |
prop_mo_ra=−77.94<ref name="vanLeeuwen2007"/> | |
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prop_mo_dec= |
prop_mo_dec= 100.83<ref name="vanLeeuwen2007"/> | |
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parallax=14.58| |
parallax=14.58 | |
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p_error=0.51| |
p_error=0.51 | |
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parallax_footnote =<ref name="vanLeeuwen2007"/> | |
parallax_footnote =<ref name="vanLeeuwen2007"/> | |
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absmag_v=2.53<ref name=aaa361_614/> }} |
absmag_v=2.53<ref name=aaa361_614/> }} |
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Simbad=HD+131041 |
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{{starbox sources|HIP|CCDM|HR}} |
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Simbad=ADS+9406 }} |
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'''39 Boötis''' ( |
'''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. |
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<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> |
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Revision as of 23:28, 11 March 2017
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] |
Distance | 224 ± 8 ly (69 ± 2 pc) |
Absolute magnitude (MV) | 2.53[5] |
Details | |
Mass | 1.43[5] M☉ |
Rotational velocity (v sin i) | 161.0[5] km/s |
Other designations | |
Database references | |
SIMBAD | data |
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
- ^ 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.
- ^ a b Haggkvist, L.; Oja, T. "Results of BV photometry 1969-70 (Uppsala refractor)". Private Communication. SIMBAD. Bibcode:1970Priv.........0H.
- ^ 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.
- ^ 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.
- ^ 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 |