Coord 2000 | 19264+4928 | Discov num | YSC 134 | Comp | Coord arcsec 2000 | 19 26 25.98 +49 27 55.1 | |||||
Date first | 2008 | Date last | 2015 | Obs | 15 | ||||||
Pa first | 202 | Pa last | 49.6 | P.A. Now (θ) | 49.6° | ||||||
Sep first | 0.0 | Sep last | 0.024 | Sep. Now (ρ) | 0.024" | ||||||
Mag pri | 8.40 | Mag sec | 9.40 | delta mag (ΔM) | 1 | Spectral class | K2V+K4.5V (yellow-orange/yellow-orange) | ||||
Pri motion ra | +457 | Sec motion ra | |||||||||
Pri motion dec | +714 | Sec motion dec | |||||||||
Notes | N O (See Notes, Orbital solution) |
Name | HD 183255 | Constellation | Cygnus | HIP | 95575 | Tycho2 | 3551-01452-1 | ||||
HD | 183255 | GL | GJ 1237 | BD | BD+49 3009 | Distance | 25.01 | ||||
Distance ly | 81.58 |
Period (P) | 0.45678y | ± 0.000008 | Periastron (T) | 2012.44y | ± 0.000257 | Semi-major axis (a) | 0.0273a | ± 0.0005 |
Eccentricity (e) | 0.13698 | ± 0.00031 | Inclination (i) | 136° | ± 1 | Longitude of periastron (ω) | 243.2° | ± 0.016 |
Node (Ω) | 23.5° | ± 1 | Notes | n | Reference | Doc2018h | ||
Equinox | 2000 | Last observation | 2015 | Grade | 2 | (1=Definitive, 9=Indet.) |
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Note: Theta is PA, Rho is Sep. For yearly orbits, data refer to Jan 1st. |
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Measures: green=micrometric, blue=interferometric, purple=photographic |
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discov_num | notes | refcode |
YSC 134 | Metal-poor SB2, spectroscopic orbit published by Tokovinin (1991). | Tok1991 |
An astrometric orbit was deduced from Hipparcos data by Jancart et al. | Jnc2005 | |
(2005). The period derived for the visual orbit matches both the | ||
spectroscopic and astrometric solutions within the uncertainty, and | ||
other orbital parametrs are in reasonable agreement with the Tokovinin | ||
solution. The updated Hipparcos parallax (39.98 +/- 0.73 mas), | ||
combined with the orbit, yields a mass sum of 2.0 +/- 0.3 Msun. The | ||
composite spectral type is K3V; a magnitude difference of 0.8 mags | ||
makes the component spectral types roughly K1V + K4V, which suggests | ||
a mass sum of 1.2-1.5 Msun, accounting for the lower metallicity. | Hor2012b | |
For the Horch et al. (2015) combined solution, spectroscopic elements | ||
are fixed to those of Halbwachs et al. (2012). Assigned spectral | HJL2012 | |
types are K2V and K4.5V; derived masses 0.74 and 0.68 Msun. | Hor2015 | |
Orbital parallax is 42.01 +/- 1.08 mas. Mass of the primary is | ||
0.695 +/- 0.066 \msun. Mass of the secondary is 0.621 +/- 0.058 \msun. | Doc2018h |
refcode | metd | author | reference |
Doc2018h | orb - | Docobo, J.A., Campo, P.P., Gomez, J. & Horch, E.P. | 2018AJ....156..185D |
Doc2018h | +not | AJ 156, 185, 2018 | |
HJL2012 | orb - | Halbwachs, J.L., Arenou, F., Famaey, B., et al. | . |
HJL2012 | SF2A-2012: Proc. Annual Meeting of the French Society of Astronomy & Astrophysics | ||
HJL2012 | 87, ed. S. Boissier et al. (Paris: Soc. Francaise d'Astron. et d'Astrop.) | ||
Hor2012b | S j | Horch, E.P., Howell, S.B., Everett, M.E., & Ciardi, D.R. | 2012AJ....144..165H |
Hor2012b | +orb | AJ 144, 165, 2012 | |
Hor2015 | S j | Horch, E.P., van Altena, W.F., Demargue, P., Howell, S.B., Everett, M.E., | 2015AJ....149..151H |
Hor2015 | +orb | Ciardi, D.R., Teske, J.K., Henry, T.J., & Winters, J.G. | |
Hor2015 | AJ 149, 151, 2015 | ||
Jnc2005 | orb - | Jancart, S., Jorrisen, A., Babusiaux, C., & Pourbaix, D. | 2005A&A...442..365J |
Jnc2005 | A&A 442, 365, 2005 | ||
Tok1991 | orb - | Tokovinin, A.A. | 1991A&AS...91..497T |
Tok1991 | A&AS 91, 497, 1991 |
idgroup | discov | author |
1 | YSC | Yale-Southern Connecticut (from additional DD list - see HOR) |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
19264+4928 | YSC 134 | 2010 | 2 | 51 | 0.0 | 8.40 | 9.40 | K3V | D | 192625.57+492748.9 | |
19264+4928 | YSC 134 | 2012 | 5 | 200 | 0.0 | 8.40 | 9.40 | K3V | D | 192625.57+492748.9 | |
19264+4928 | YSC 134 | 2014 | 11 | 272 | 0.0 | 8.40 | 9.40 | K2V K4.5V | NO | 192625.57+492748.9 | |
19264+4928 | YSC 134 | 2015 | 15 | 50 | 0.0 | 8.40 | 9.40 | K2V+K4.5V | NO | 192625.98+492755.1 |
Click on the map to see the double of your interest. Pass over with the mouse cursor to display the catalog designation. |
Click on the map to see the double of your interest. Pass over with the mouse cursor to display the catalog designation. |
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A | |
B | pa=37.4° sep=0.02" |
Componente originario normalizzato | AB | Name | HD 183255 | Coord arcsec 2000 | 192625.98+492755.1 | Mag | 8.4 | ||||
Spectral class | K2V (yellow-orange) | PmRA | 457.00 | PmDE | 714.0 | HIP | 95575 | ||||
Tycho2 | 3551-01452-1 | HD | 183255 | BD | BD+49 3009 |
Tycho2 | 3551-01452-1 | Pflag | RAmdeg | 291.60826472 | DEmdeg | 49.46530948 | |||||
PmRA | 456.7 | PmDE | 713.0 | E RAmdeg | 7 | E DEmdeg | 6 | ||||
E pmRA | 1.3 | E pmDE | 1.3 | EpRAm | 1990.96 | EpDEm | 1991.29 | ||||
Num | 9 | Q RAmdeg | 0.3 | Q DEmdeg | 1.2 | Q pmRA | 0.3 | ||||
Q pmDE | 1.2 | BTmag | 9.235 | E BTmag | 0.019 | VTmag | 8.146 | ||||
E VTmag | 0.012 | Prox | 999 | TYC | T | HIP | 95575 | ||||
CCDM | RAdeg | 291.60660167 | DEdeg | 49.46364778 | EpRA 1990 | 1.48 | |||||
EpDE 1990 | 1.61 | E RAdeg | 7.3 | E DEdeg | 6.3 | Posflg | |||||
Corr | 0.1 |
Catalog | H | HIP | 95575 | Proxy | RAhms | 19 26 25.57 | |||||
DEdms | +49 27 48.9 | Vmag | 8.01 | VarFlag | R Vmag | H | |||||
RAdeg | 291.607 | DEdeg | 49.4636 | AstroRef | Plx | 39.73 | |||||
CCDM | N CCDM | Nsys | Ncomp | 1 | |||||||
MultFlag | X | Source | Qual | M HIP | |||||||
Theta | Rho | HD | 183255 | BD | BD+49 3009 | ||||||
CD | CP | Dm number | +49 3009 | VIred | 0.97 | ||||||
SpType | K3V | R SpType | Coord arcsec 2000 | 192625.57+492748.9 |
HIP | 95575 | Sn | 5 | So | 2 | Nc | 1 | ||||
RArad | 5.0894945494 | DErad | 0.8633022531 | Plx | 39.98 | PmRA | 457.1 | ||||
PmDE | 713.96 | E RArad | 0.68 | E DErad | 0.61 | E Plx | 0.73 | ||||
E pmRA | 0.82 | E pmDE | 0.77 | Hpmag | 8.1541 | E Hpmag | 0.0013 | ||||
SHp | 0.013 | VA | 0 | BV | 0.929 | E BV | 0.009 | ||||
VI | 0.97 |
Componente originario normalizzato | AB | Coord arcsec 2000 | 192625.98+492755.1 | Mag | 9.4 | Spectral class | K4.5V (yellow-orange) | ||||
Calc delta mag | 1 | Calc coord | yes |