HATS-39b, HATS-40b, HATS-41b, and HATS-42b: three inflated hot Jupiters and a super-Jupiter transiting F stars. Issue 3 (20th March 2018)
- Record Type:
- Journal Article
- Title:
- HATS-39b, HATS-40b, HATS-41b, and HATS-42b: three inflated hot Jupiters and a super-Jupiter transiting F stars. Issue 3 (20th March 2018)
- Main Title:
- HATS-39b, HATS-40b, HATS-41b, and HATS-42b: three inflated hot Jupiters and a super-Jupiter transiting F stars
- Authors:
- Bento, J
Hartman, J D
Bakos, G Á
Bhatti, W
Csubry, Z
Penev, K
Bayliss, D
de Val-Borro, M
Zhou, G
Brahm, R
Espinoza, N
Rabus, M
Jordán, A
Suc, V
Ciceri, S
Sarkis, P
Henning, T
Mancini, L
Tinney, C G
Wright, D J
Durkan, S
Tan, T G
Lázár, J
Papp, I
Sári, P - Abstract:
- Abstract: We report the discovery of four transiting hot Jupiters from the HATSouth survey: HATS-39b, HATS-40b, HATS-41b, and HATS-42b. These discoveries add to the growing number of transiting planets orbiting moderately bright (12.5 ≲ V ≲ 13.7) F dwarf stars on short (2-5 d) periods. The planets have similar radii, ranging from $1.33^{+0.29}_{-0.20}$ R J for HATS-41b to $1.58^{+0.16}_{-0.12}$ R J for HATS-40b. Their masses and bulk densities, however, span more than an order of magnitude. HATS-39b has a mass of 0.63 ± 0.13 M J, and an inflated radius of 1.57 ± 0.12 R J, making it a good target for future transmission spectroscopic studies. HATS-41b is a very massive 9.7 ± 1.6 M J planet and one of only a few hot Jupiters found to date with a mass over 5 M J . This planet orbits the highest metallicity star ([Fe/H] = 0.470 ± 0.010) known to host a transiting planet and is also likely on an eccentric orbit. The high mass, coupled with a relatively young age ($1.34^{+0.31}_{-0.51}$ Gyr) for the host star, is a factor that may explain why this planet's orbit has not yet circularized.
- Is Part Of:
- Monthly notices of the Royal Astronomical Society. Volume 477:Issue 3(2018)
- Journal:
- Monthly notices of the Royal Astronomical Society
- Issue:
- Volume 477:Issue 3(2018)
- Issue Display:
- Volume 477, Issue 3 (2018)
- Year:
- 2018
- Volume:
- 477
- Issue:
- 3
- Issue Sort Value:
- 2018-0477-0003-0000
- Page Start:
- 3406
- Page End:
- 3423
- Publication Date:
- 2018-03-20
- Subjects:
- techniques: photometric -- techniques: spectroscopic -- stars: individual: HATS-39, HATS-40, HATS-41, HATS-42 -- stars: individual: GSC 6550-00341, GSC 6533-01514, GSC 6530-01596, GSC 7107-03973 -- planetary systems
Astronomy -- Periodicals
Periodicals
520.5 - Journal URLs:
- http://mnras.oxfordjournals.org/ ↗
http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966 ↗
http://www.blackwell-synergy.com/issuelist.asp?journal=mnr ↗
http://www.blackwell-synergy.com/loi/mnr ↗
http://ukcatalogue.oup.com/ ↗ - DOI:
- 10.1093/mnras/sty726 ↗
- Languages:
- English
- ISSNs:
- 0035-8711
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
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