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26 Sep 2019: There are few disks detected around the less massiveM stars, but this is likely an observational bias and there is no evidence as yet to say. ... However, ongoing interferometric surveys have shown that excesses at 0.1-1% levels are more common, and

7 Jan 2014: 2013) andthe Fomalhaut tertiary system (Kennedy et al. 2013a). 2.5. Correlation with Exoplanet Populations. ... Dust (and planetesimals) were assumed to be a mixture ofastrosilicate and water ice in equal mass fractions.

22 Mar 2024: Q2) What fraction of terrestrial exoplanets provide (surface) conditions so that liquid water and life as we know it could in principle exist? ... has been growing at a breathtaking speed: to date we know more than 5000 exoplanets and exoplanet

20 Aug 2021: Q2) What fraction of terrestrial exoplanets provide (surface) conditions so that liquid water and life as we know it could in principle exist? ... has been growing at a breathtaking speed: to date we know more than 5000 exoplanets and exoplanet

22 Mar 2024: a) Open air deposits may exist above the local water table, whereasdilute deposits lie in it. ... Nature 459, 239–242 (2009). [3] Rimmer, P. B. et al. The origin of RNA precursors on exoplanets.

5 Apr 2011: 0.4. 0.8 200 Myr. Semimajor Axis (AU). Ecc. entr. icity. Log(Water Mass Fraction). ... Colors denote water content, assuming a Solar System-like initial distribution (Raymond et al.

12 Oct 2021: Yet, such low levels are important not only for their astrophysical context (i.e.,. ... Blommaert, C. Waelkens, L. B. F. M. Waters, B. Vandenbussche,M. Min, G.

23 Oct 2019: 1 Taken on 28 November 2018 from the exoplanet.eu database (Schneideret al. ... circles are known exoplanets for 0.6 1.4M stars (from the exoplanet.eu database on 28 November 2018, Schneider et al.

15 May 2018: Exoplanet recycling in massive white-dwarf debris discs. R. van Lieshout,1? Q. ... This atmospheric metalpollution is a much more common phenomenon than the IR excess,?

15 Mar 2016: Suchimpacts would have been quite common in the late stages of terrestrial planetformation (e.g. ... Exoplanet spinsare already measurable in observations of the velocity profile from lines intheir atmospheres (Snellen et al.

19 Jan 2012: 0.4. 0.8 200 Myr. Semimajor Axis (AU). Ecc. entr. icity. Log(Water Mass Fraction). ... The inner planet is wet:it accreted a small amount of water from material that originated.

21 Jan 2014: 2013), and in addition hosts an enig-matic exoplanet, Fomalhaut b (Kalas et al. ... R., & Crockett,N. 2008, ApJS, 179, 423. Decin, G., Dominik, C., Waters, L.

2 Jul 2014: 3 Databases of exoplanet properties are maintained athttp://exoplanet.eu and http://exoplanets.org. 1. ... 1999; Fischer et al. 2014). Recentresults from an analysis of microlensing surveys suggest thatalmost all stars may have one or more exoplanets,

22 Mar 2024: 2021)or the GPI-GPIES survey (Gemini Planet Imager Exoplanet Sur-vey, Nielsen et al. ... Dahlqvist et al.: SHARDDS Survey. minosity above 104) and because they were not yet resolved inscattered light.

23 Nov 2021: System comets/asteroids? — Sect. 44. How do water and ice abundances within the disk. ... can increase the mass loss by a factor ofone hundred, assuming common X-ray luminosities.

8 Jan 2015: Cherry Lane, Tucson, AZ, 85721, USA. Rafael Millan-GabetNASA Exoplanet Science Institute, California Institute of Technology, Pasadena, CA, 91125, USA. ... LBTIis still in commissioning, so the final dependence of nulldepth on target brightness is not

27 Jan 2016: 5NASA Goddard Space Flight Center, Exoplanets & Stellar Astrophysics Laboratory, Code 667, Greenbelt, MD 20771, USA6Large Binocular Telescope Observatory, University of Arizona, 933 N. ... 2014). To minimize non-common patherrors, we split the

10 Nov 2021: 6 Centre for Exoplanets and Habitability, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK. ... studies of ice-bearing asteroids in the Solar System show that while retaining water ice in the.

10 Mar 2020: imaging search for Earth-like exoplanets, but more precise constraints are still required, in particular. ... the environmental conditions of potential rocky planets. (cometary bombardment, delivery of water; Kral et al.

20 Nov 2019: 4Centre for Exoplanets and Habitability, University of Warwick, Gibbet Hill Road, Coventry, CV4 7AL, UK5Instituto Nacional de Astrof́ısica, Óptica y Electrónica, Luis Enrique Erro 1, Sta. ... The morphology and dynamics of a disk encode information

7 Oct 2016: Herewe took the known exoplanets from the NASA exoplanetarchive 1 on 25 Feb 2016. ... This does not necessarily include all known exoplanets,but serves to illustrate the main features of the exoplanetpopulation.

23 Jun 2009: Tentative evidence for a common position angle for the dust at 1.7AU with that at 150AU aroundη Corvi, which mightbe expected if the hot dust is fed from the outer ... Butleret al. 2006). Debris disc studies are therefore typically comple-mentary to

19 Apr 2006: to theobservations of debris disks around other stars; and e) how these new results impactour assessment of whether systems like our own are common or rare compared to theensemble of normal ... notplanetary systems like our own are common or rare in

5 May 2017: This could be due to common favourable forming conditions forrocky planets close in and planetesimals at large radii. ... Debris discs at tens of AU arefairly common around FGK stars, with occurrence rates of at least 20% (e.g., Su et al.

22 Mar 2024: It has been questionedwhether M-dwarf discs are simply less common than earlier types, or whether the low detection rate derives from the wavelengthsand sensitivities available to those studies. ... Thereare only eight nearby M-dwarf discs published in

15 Oct 2020: 1 INTRODUCTION. We are observing ever-increasing numbers of exoplanets (Kalteneg-ger 2017; Defrère et al. ... as left-overplanetesimals), the latter of which has not yet been studied in thecontext of their effect on the Earth’s atmosphere.

23 Feb 2012: sized components), as demonstrated by the presence ofsignificant amounts of non-refractory water-ice in the ejecta(Lisse et al. ... pyrrohtite; carbonates such as magnesite andsiderite; water-gas and ice; amorphous carbon (and potentiallynative Fe:Ni);

24 Oct 2015: al., 2014; Keto et al., 2008), butare not yet contaminated by molecular lines as is often the case in the ALMArange at > 100 GHz. ... These structures can be interpreted as the result of the gravitationalinteraction between as-of-yet unseen giant planets

22 Mar 2024: Thismodel, however, has not yet been tested against the measured COgas masses and constraints on its composition. ... 2021), theoptically thin nature of debris discs means most molecules will beshort-lived and scarce.

29 Apr 2021: est. The wide orbits of Fomalhaut’s stellar companions constitutesufficient angular momentum to preclude a common protostellarcore fragmentation scenario. ... Themagnitude of the orbital period

31 Jul 2018: Thus, it is not yet clear how farfrom their stars planets can form. ... HD 92945 (Golimowski. 1 http://exoplanet.eu/. et al. 2011) and HD 131835 (Feldt et al.

29 Sep 2022: 7AL, UK5Centre for Exoplanets and Habitability, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK6California Institute of Technology, Pasadena, CA 91125, USA7IPAC-NASA Exoplanet Science Institute Pasadena, CA 91125, USA8Department

20 Feb 2024: Victor Jara 3659, Santiago 9170124, Chile 13 Millennium Nucleus on Young Exoplanets and their Moons (YEMS), Santiago 9170124, Chile 14 Center for Interdisciplinary Research in Astrophysics and Space Exploration (CIRAS), Universidad ... the largest bodies

25 Oct 2022: 7Departamento de Física, Universidad de Santiago de Chile, Av. Ecuador 3493, Estación Central, Santiago, Chile8Millennium Nucleus on Young Exoplanets and their Moons (YEMS), Chile. ... Such planets could beembedded in the disk and have cleared gaps (>

8 Jul 2020: USA4Department of Physics, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK5Centre for Exoplanets and Habitability, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK6Max Planck Institute for Astronomy, ... ABSTRACTGas detection

16 Jul 2021: Suchcircumstellar dust and the implied planetesimals collectively form. 1 http://exoplanet.eu. 2020TheAuthors. ... 2016). This component is yet to be resolved, butmaybe in close proximity to the exo-Jupiter q1 Erib.

18 Oct 2014: 2NASA Exoplanet Science Center, California Institute of Technology, 770 South Wilson Avenue, Pasadena CA 91125, USA. ... 5NASA Goddard Space Flight Center, Exoplanets and Stellar Astrophysics Laboratory, Code 667, Greenbelt, MD 20771,.

11 Jul 2019: Wyatt11Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK2Department of Physics, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK3Centre for Exoplanets and Habitability, University of Warwick,

10 Feb 2021: Tőravere, Estonia4Department of Physics, University of Warwick, Coventry, CV4 7AL, UK5Centre for Exoplanets and Habitability, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL, UK6European Southern Observatory, Karl-Schwarzschild-Strasse 2,