HAT-P-16b: A 4 M J planet transiting a bright star on an eccentric orbit

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Standard

HAT-P-16b : A 4 M J planet transiting a bright star on an eccentric orbit. / Buchhave, Lars A.; Bakos, G. A.; Hartman, J. D.; Torres..[et al.], G.

I: Astrophysical Journal, Bind 720, Nr. 2, 17.08.2010, s. 1118-1125.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Buchhave, LA, Bakos, GA, Hartman, JD & Torres..[et al.], G 2010, 'HAT-P-16b: A 4 M J planet transiting a bright star on an eccentric orbit', Astrophysical Journal, bind 720, nr. 2, s. 1118-1125. https://doi.org/10.1088/0004-637X/720/2/1118

APA

Buchhave, L. A., Bakos, G. A., Hartman, J. D., & Torres..[et al.], G. (2010). HAT-P-16b: A 4 M J planet transiting a bright star on an eccentric orbit. Astrophysical Journal, 720(2), 1118-1125. https://doi.org/10.1088/0004-637X/720/2/1118

Vancouver

Buchhave LA, Bakos GA, Hartman JD, Torres..[et al.] G. HAT-P-16b: A 4 M J planet transiting a bright star on an eccentric orbit. Astrophysical Journal. 2010 aug. 17;720(2):1118-1125. https://doi.org/10.1088/0004-637X/720/2/1118

Author

Buchhave, Lars A. ; Bakos, G. A. ; Hartman, J. D. ; Torres..[et al.], G. / HAT-P-16b : A 4 M J planet transiting a bright star on an eccentric orbit. I: Astrophysical Journal. 2010 ; Bind 720, Nr. 2. s. 1118-1125.

Bibtex

@article{984616c8421d4c9ba46594d3589fb788,
title = "HAT-P-16b: A 4 M J planet transiting a bright star on an eccentric orbit",
abstract = "We report the discovery of HAT-P-16b, a transiting extrasolar planet orbiting the V = 10.8 mag F8 dwarf GSC 2792-01700, with a period P = 2.775960 ± 0.000003 days, transit epoch Tc = 2455027.59293 ± 0.00031 (BJD10), and transit duration 0.1276 ± 0.0013 days. The host star has a mass of 1.22 ± 0.04 M , radius of 1.24 ± 0.05 R , effective temperature 6158 ± 80 K, and metallicity [Fe/H] = +0.17 ± 0.08. The planetary companion has a mass of 4.193 ± 0.094 M J and radius of 1.289 ± 0.066 R J, yielding a mean density of 2.42 ± 0.35 g cm–3. Comparing these observed characteristics with recent theoretical models, we find that HAT-P-16b is consistent with a 1 Gyr H/He-dominated gas giant planet. HAT-P-16b resides in a sparsely populated region of the mass-radius diagram and has a non-zero eccentricity of e = 0.036 with a significance of 10s. ",
author = "Buchhave, {Lars A.} and Bakos, {G. A.} and Hartman, {J. D.} and {Torres..[et al.]}, G.",
year = "2010",
month = aug,
day = "17",
doi = "10.1088/0004-637X/720/2/1118",
language = "English",
volume = "720",
pages = "1118--1125",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - HAT-P-16b

T2 - A 4 M J planet transiting a bright star on an eccentric orbit

AU - Buchhave, Lars A.

AU - Bakos, G. A.

AU - Hartman, J. D.

AU - Torres..[et al.], G.

PY - 2010/8/17

Y1 - 2010/8/17

N2 - We report the discovery of HAT-P-16b, a transiting extrasolar planet orbiting the V = 10.8 mag F8 dwarf GSC 2792-01700, with a period P = 2.775960 ± 0.000003 days, transit epoch Tc = 2455027.59293 ± 0.00031 (BJD10), and transit duration 0.1276 ± 0.0013 days. The host star has a mass of 1.22 ± 0.04 M , radius of 1.24 ± 0.05 R , effective temperature 6158 ± 80 K, and metallicity [Fe/H] = +0.17 ± 0.08. The planetary companion has a mass of 4.193 ± 0.094 M J and radius of 1.289 ± 0.066 R J, yielding a mean density of 2.42 ± 0.35 g cm–3. Comparing these observed characteristics with recent theoretical models, we find that HAT-P-16b is consistent with a 1 Gyr H/He-dominated gas giant planet. HAT-P-16b resides in a sparsely populated region of the mass-radius diagram and has a non-zero eccentricity of e = 0.036 with a significance of 10s.

AB - We report the discovery of HAT-P-16b, a transiting extrasolar planet orbiting the V = 10.8 mag F8 dwarf GSC 2792-01700, with a period P = 2.775960 ± 0.000003 days, transit epoch Tc = 2455027.59293 ± 0.00031 (BJD10), and transit duration 0.1276 ± 0.0013 days. The host star has a mass of 1.22 ± 0.04 M , radius of 1.24 ± 0.05 R , effective temperature 6158 ± 80 K, and metallicity [Fe/H] = +0.17 ± 0.08. The planetary companion has a mass of 4.193 ± 0.094 M J and radius of 1.289 ± 0.066 R J, yielding a mean density of 2.42 ± 0.35 g cm–3. Comparing these observed characteristics with recent theoretical models, we find that HAT-P-16b is consistent with a 1 Gyr H/He-dominated gas giant planet. HAT-P-16b resides in a sparsely populated region of the mass-radius diagram and has a non-zero eccentricity of e = 0.036 with a significance of 10s.

U2 - 10.1088/0004-637X/720/2/1118

DO - 10.1088/0004-637X/720/2/1118

M3 - Journal article

VL - 720

SP - 1118

EP - 1125

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

ER -

ID: 32930028