From Wikipedia, the free encyclopedia
Star in the constellation Ursa Major
HAT-P-3 , is a
metal-rich
K5 dwarf star located about 441
light-years away in the
constellation
Ursa Major . At a
magnitude of about 11.5 it is not visible to the
naked eye but is visible in a small to medium-sized
amateur telescope . It is believed to be a relatively young star and has a slightly enhanced level of
chromospheric activity .
[7]
[9]
The star HAT-P-3 is named Dombay . The name was selected in the
NameExoWorlds campaign by
Russia , during the 100th anniversary of the
IAU .
Dombay is a resort region in the North
Caucasus mountains.
[10]
[11]
Planetary system
This star is home to the
extrasolar planet
HAT-P-3b , later named Teberda , discovered by the
HATNet Project using the
transit method .
[7]
See also
References
^ Roman, Nancy G. (1987).
"Identification of a Constellation From a Position" . Publications of the Astronomical Society of the Pacific . 99 (617): 695–699.
Bibcode :
1987PASP...99..695R .
doi :
10.1086/132034 .
Vizier query form
^
a
b
c
d Vallenari, A.; et al. (Gaia collaboration) (2023).
"Gaia Data Release 3. Summary of the content and survey properties" . Astronomy and Astrophysics . 674 : A1.
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 Droege, Thomas F.; et al. (2006). "TASS Mark IV Photometric Survey of the Northern Sky". The Publications of the Astronomical Society of the Pacific . 118 (850): 1666–1678.
arXiv :
astro-ph/0610529 .
Bibcode :
2006PASP..118.1666D .
doi :
10.1086/510197 .
JSTOR
10.1086/510197 .
S2CID
11716917 .
Vizier catalog entry
^
a
b
c
d
e
f
g
h Mancini, L.; Esposito, M.; Covino, E.; Southworth, J.; Biazzo, K.; Bruni, I.; Ciceri, S.; Evans, D.; Lanza, A. F.; Poretti, E.; Sarkis, P.; Smith, A. M. S.; Brogi, M.; Affer, L.; Benatti, S.; Bignamini, A.; Boccato, C.; Bonomo, A. S.; Borsa, F.; Carleo, I.; Claudi, R.; Cosentino, R.; Damasso, M.; Desidera, S.; Giacobbe, P.; González-Álvarez, E.; Gratton, R.; Harutyunyan, A.; Leto, G.; et al. (2018). "The GAPS programme with HARPS-N at TNG". Astronomy & Astrophysics . 613 : A41.
arXiv :
1802.03859 .
Bibcode :
2018A&A...613A..41M .
doi :
10.1051/0004-6361/201732234 .
S2CID
73565379 .
^
a
b
"TYC 3466-819-1" .
SIMBAD .
Centre de données astronomiques de Strasbourg . Retrieved 2013-10-29 .
^
a
b
c Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006).
"The Two Micron All Sky Survey (2MASS)" . The Astronomical Journal . 131 (2): 1163–1183.
Bibcode :
2006AJ....131.1163S .
doi :
10.1086/498708 .
ISSN
0004-6256 .
S2CID
18913331 .
Vizier catalog entry
^
a
b
c
d Torres, G.; et al. (2007).
"HAT-P-3b: A Heavy-Element-rich Planet Transiting a K Dwarf Star" . The Astrophysical Journal Letters . 666 (2): L121–L124.
arXiv :
0707.4268 .
Bibcode :
2007ApJ...666L.121T .
doi :
10.1086/521792 .
S2CID
16549542 .
^
a
b
c Chan, Tucker; et al. (2011). "The Transit Light-curve Project. XIV. Confirmation of Anomalous Radii for the Exoplanets TrES-4b, HAT-P-3b, and WASP-12b". The Astronomical Journal . 141 (6). 179.
arXiv :
1103.3078 .
Bibcode :
2011AJ....141..179C .
doi :
10.1088/0004-6256/141/6/179 .
S2CID
56378813 .
^ Todorov, Kamen O.; et al. (2013). "Warm Spitzer Photometry of Three Hot Jupiters: HAT-P-3b, HAT-P-4b and HAT-P-12b". The Astrophysical Journal . 770 (2). 102.
arXiv :
1305.0833 .
Bibcode :
2013ApJ...770..102T .
doi :
10.1088/0004-637X/770/2/102 .
S2CID
51509956 .
^
"Approved names" . NameExoworlds . Archived from
the original on 2019-12-19. Retrieved 2020-01-02 .
^
"International Astronomical Union | IAU" . www.iau.org . Retrieved 2020-01-02 .
^ Bonomo, A. S.; et al. (2017). "The GAPS Programme with HARPS-N at TNG . XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets". Astronomy and Astrophysics . 602 . A107.
arXiv :
1704.00373 .
Bibcode :
2017A&A...602A.107B .
doi :
10.1051/0004-6361/201629882 .
S2CID
118923163 .
External links