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F-type main-sequence star; Triangulum.
HD 11007 (LTT 10624; HR 523 ) is a probable
astrometric binary
[13] located in the northern
constellation
Triangulum . The primary is faintly visible to the
naked eye as a whitish-yellow-hued
star with an
apparent magnitude of 5.81.
[2] The system is located relatively close at a distance of 90.4
light-years based on
Gaia DR3
parallax measurements
[1] and it is drifting closer with a heliocentric
radial velocity of −24.4
km/s .
[4] At its current distance, HD 11007's brightness is diminished by an
interstellar extinction of 0.09
magnitudes
[14] and it has an
absolute magnitude of +3.56.
[5] It is moving relatively fast across the
celestial sphere ,
[15] having a high
proper motion of 341 mas/yr.
[1]
The primary has a
stellar classification of F8 V,
[3] indicating that it is an ordinary
F-type main-sequence star that is generating energy via
hydrogen fusion at its
core . However, it is slightly evolved, being 1.62 magnitudes above the
zero age main sequence .
[16] It has 111% the
mass of the Sun
[6] and a slightly enlarged
radius 1.67 times that of the
Sun .
[7] It is slightly over luminous for its class, radiating 3.23 times the
luminosity of the Sun
[1] from its
photosphere at an
effective temperature of 6,060
K .
[7] HD 11007 A is metal deficient with an
iron abundance that is 63.1% solar
[9] and it spins modestly with a somewhat constrained
projected rotational velocity of approximately 5
km/s .
[10] The system is estimated to be 6.6
billion years old; it was suspected to be part of the
thick disk population
[11] but is now considered to be one of the older members of the
thin disk population .
[17]
References
^
a
b
c
d
e
f
g
h Vallenari, A.; et al. (Gaia collaboration) (2023).
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arXiv :
2208.00211 .
Bibcode :
2023A&A...674A...1G .
doi :
10.1051/0004-6361/202243940 .
S2CID
244398875 .
Gaia DR3 record for this source at
VizieR .
^
a
b
c
d Imagawa, Fumihiko (February 1967).
"Observational Results of Three-color Photometry for F-type Stars (II)" . Memoirs of the College of Science, University of Kyoto. Series A . 31 (2): 93–100.
^
a
b Harlan, E. A. (June 1974).
"MK classifications for F-and G-type stars. 3" . The Astronomical Journal . 79 : 682.
Bibcode :
1974AJ.....79..682H .
doi :
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ISSN
0004-6256 .
^
a
b Gontcharov, G. A. (November 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 .
eISSN
1562-6873 .
ISSN
1063-7737 .
S2CID
119231169 .
^
a
b Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters . 38 (5): 331–346.
arXiv :
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Bibcode :
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doi :
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^
a
b Lambert, David L.; Reddy, Bacham E. (2004).
"Lithium abundances of the local thin disc stars" . Monthly Notices of the Royal Astronomical Society . 349 (2): 757–767.
arXiv :
astro-ph/0401259 .
Bibcode :
2004MNRAS.349..757L .
doi :
10.1111/j.1365-2966.2004.07557.x .
S2CID
118931004 .
^
a
b
c
d Masana, E.; Jordi, C.; Ribas, I. (10 April 2006).
"Effective temperature scale and bolometric corrections from 2MASS photometry" . Astronomy & Astrophysics . 450 (2): 735–746.
arXiv :
astro-ph/0601049 .
Bibcode :
2006A&A...450..735M .
doi :
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eISSN
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ISSN
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S2CID
15278668 .
^ Aguilera-Gómez, Claudia; Ramírez, Iván; Chanamé, Julio (June 2018).
"Lithium abundance patterns of late-F stars: an in-depth analysis of the lithium desert" . Astronomy & Astrophysics . 614 : A55.
arXiv :
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Bibcode :
2018A&A...614A..55A .
doi :
10.1051/0004-6361/201732209 .
eISSN
1432-0746 .
ISSN
0004-6361 .
S2CID
62799777 .
^
a
b Mishenina, T; Pignatari, M; Gorbaneva, T; Travaglio, C; Côté, B; Thielemann, F-K; Soubiran, C (October 21, 2019).
"Enrichment of the Galactic disc with neutron-capture elements: Mo and Ru" . Monthly Notices of the Royal Astronomical Society . 489 (2): 1697–1708.
arXiv :
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Bibcode :
2019MNRAS.489.1697M .
doi :
10.1093/mnras/stz2202 .
ISSN
0035-8711 .
S2CID
199511206 .
^
a
b Balachandran, Suchitra (May 1990).
"Lithium depletion and rotation in main-sequence stars" . The Astrophysical Journal . 354 . American Astronomical Society: 310.
Bibcode :
1990ApJ...354..310B .
doi :
10.1086/168691 .
ISSN
0004-637X .
S2CID
120769481 .
^
a
b Liu, Wilson M.; Chaboyer, Brian (December 2000).
"The Relative Age of the Thin and Thick Galactic Disks" . The Astrophysical Journal . 544 (2): 818–829.
arXiv :
astro-ph/0007193 .
Bibcode :
2000ApJ...544..818L .
doi :
10.1086/317231 .
ISSN
0004-637X .
S2CID
14270478 .
^
"HD 11007" .
SIMBAD .
Centre de données astronomiques de Strasbourg .
^ Eggleton, P. P.; Tokovinin, A. A. (11 September 2008).
"A catalogue of multiplicity among bright stellar systems" . Monthly Notices of the Royal Astronomical Society . 389 (2): 869–879.
arXiv :
0806.2878 .
Bibcode :
2008MNRAS.389..869E .
doi :
10.1111/j.1365-2966.2008.13596.x .
eISSN
1365-2966 .
ISSN
0035-8711 .
S2CID
14878976 .
^ Gontcharov, George A.; Mosenkov, Aleksandr V. (28 September 2017).
"Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars" . Monthly Notices of the Royal Astronomical Society . 472 (4): 3805–3820.
arXiv :
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Bibcode :
2017MNRAS.472.3805G .
doi :
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eISSN
1365-2966 .
ISSN
0035-8711 .
S2CID
118879856 .
^ Ivanov, G. A. (June 2002). "Cross-identifications of stars with high proper motion". Kinematika i Fizika Nebesnykh Tel . 18 : 287–288.
Bibcode :
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ISSN
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^ Nordström, B.; Mayor, M.; Andersen, J.; Holmberg, J.; Pont, F.; Jørgensen, B. R.; Olsen, E. H.; Udry, S.; Mowlavi, N. (16 April 2004).
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arXiv :
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Bibcode :
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doi :
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eISSN
1432-0746 .
ISSN
0004-6361 .
S2CID
11027621 .
^ Mishenina, T. V.; Soubiran, C.; Kovtyukh, V. V.; Korotin, S. A. (May 2004).
"On the correlation of elemental abundances with kinematics among galactic disk stars" . Astronomy & Astrophysics . 418 (2): 551–562.
arXiv :
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doi :
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ISSN
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S2CID
17514939 .