| ALMA sheds light on planet-forming gas streams (HD 142527) | |
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Led_Zep SuperJovian
Number of posts : 721 Location : France Registration date : 2011-09-09
| Subject: ALMA sheds light on planet-forming gas streams (HD 142527) 2nd January 2013, 1:20 pm | |
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Sirius_Alpha Admin
Number of posts : 4320 Location : Earth Registration date : 2008-04-06
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 2nd January 2013, 2:12 pm | |
| Very interesting. I'm having a hard time interpreting the ALMA image(s) correctly. _________________ Caps Lock: Cruise control for 'Cool'!
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Led_Zep SuperJovian
Number of posts : 721 Location : France Registration date : 2011-09-09
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 2nd January 2013, 4:40 pm | |
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Led_Zep SuperJovian
Number of posts : 721 Location : France Registration date : 2011-09-09
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 2nd January 2013, 4:59 pm | |
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Lazarus dF star
Number of posts : 3337 Registration date : 2008-06-12
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 3rd January 2013, 4:13 pm | |
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Lazarus dF star
Number of posts : 3337 Registration date : 2008-06-12
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 9th January 2014, 1:16 pm | |
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Led_Zep SuperJovian
Number of posts : 721 Location : France Registration date : 2011-09-09
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 17th January 2014, 3:11 pm | |
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Lazarus dF star
Number of posts : 3337 Registration date : 2008-06-12
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 18th January 2014, 4:24 am | |
| This definitely seems to be a system to look out for, what with the discs around each of the two individual stars and a planet-forming circumbinary disc. | |
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Sirius_Alpha Admin
Number of posts : 4320 Location : Earth Registration date : 2008-04-06
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 28th July 2014, 8:42 pm | |
| GPI detection of circumsecondary disk. Polarized Light Imaging of the HD 142527 Transition Disk with the Gemini Planet Imager: Dust around the Close-in Companion http://arxiv.org/abs/1407.7041 - Quote :
- Because the scattering dust is likely falling onto or orbiting the companion, it is possible tht this dust contributes to the total intensity that has been directly detected at other wavelengths. If this is the case, the reported masses for the companion (0.1 - 0.4 solar masses) should be viewed as upper limits only.
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- If, on the other hand, the companion is a gas giant planet or protoplanet, then the light we see at Y band (and at other wavelengts) is dominated by the circumsecondary dust, meaning the true fractional polarisation would be small. This could indicate that the dust near the companion might then originate from the inner disk. This would suggest that dust grains from the outer disk are not following the gap-crossing gas. It might also mean that multiple planets are responsible for the observed wide disk gap, since photoevaporation is unlikely in this accreting system.
And lastly, - Quote :
- The detection of the companion and nearby dust in polarized light in just 12 minuates of integration at < 0.11" suggests that ODD in concert with ADI+PCA can be a powerful tool for detecting dust around off-axis point sources. In particular, older planets with their own circumbinary disks or rings may even be detectable by current facilities like GPI in the coming years.
(emphasis mine) _________________ Caps Lock: Cruise control for 'Cool'!
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Lazarus dF star
Number of posts : 3337 Registration date : 2008-06-12
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 9th January 2015, 3:23 am | |
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Lazarus dF star
Number of posts : 3337 Registration date : 2008-06-12
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 1st December 2015, 8:20 pm | |
| Update on the orbital properties of HD 142527 B: seems to be aligned with the inner disc and unlikely to be responsible for creating the cavity in the outer disc. Lacour et al. "An M-dwarf star in the transition disk of Herbig HD142527; Physical parameters and orbital elements" http://arxiv.org/abs/1511.09390 | |
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Led_Zep SuperJovian
Number of posts : 721 Location : France Registration date : 2011-09-09
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 5th December 2016, 6:47 pm | |
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Lazarus dF star
Number of posts : 3337 Registration date : 2008-06-12
| Subject: Re: ALMA sheds light on planet-forming gas streams (HD 142527) 27th March 2020, 12:15 pm | |
| Brittain et al. "The Planetary Luminosity Problem: 'Missing Planets' and the Observational Consequences of Episodic Accretion" https://arxiv.org/abs/2003.11980The paper suggests that the discrepancy between the occurrence rates of features in discs attributed to giant planets and the rates of detection of giant planets may be due to the majority of giant planets forming in a "cold start" process, with occasional episodes of higher-luminosity accretion. They suggest that HD 142527 B may be a super-Jupiter planet undergoing an accretion outburst rather than an M dwarf star. The full Gaia dataset should allow a mass determination to discriminate between these possibilities. | |
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| ALMA sheds light on planet-forming gas streams (HD 142527) | |
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