POLARIZED LIGHT IMAGING OF THE HD 142527 TRANSITION DISK WITH THE GEMINI PLANET IMAGER: DUST AROUND THE CLOSE-IN COMPANION
Journal Article
·
· Astrophysical Journal Letters
- Department of Terrestrial Magnetism, Carnegie Institute of Washington, 5241 Broad Branch Road, NW, Washington, DC 20015 (United States)
- Steward Observatory, The University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721 (United States)
When giant planets form, they grow by accreting gas and dust. HD 142527 is a young star that offers a scaled-up view of this process. It has a broad, asymmetric ring of gas and dust beyond ∼100 AU and a wide inner gap. Within the gap, a low-mass stellar companion orbits the primary star at just ∼12 AU, and both the primary and secondary are accreting gas. In an attempt to directly detect the dusty counterpart to this accreted gas, we have observed HD 142527 with the Gemini Planet Imager in polarized light at Y band (0.95-1.14 μm). We clearly detect the companion in total intensity and show that its position and photometry are generally consistent with the expected values. We also detect a point source in polarized light that may be spatially separated by ∼ a few AU from the location of the companion in total intensity. This suggests that dust is likely falling onto or orbiting the companion. Given the possible contribution of scattered light from this dust to previously reported photometry of the companion, the current mass limits should be viewed as upper limits only. If the dust near the companion is eventually confirmed to be spatially separated, this system would resemble a scaled-up version of the young planetary system inside the gap of the transition disk around LkCa 15.
- OSTI ID:
- 22365251
- Journal Information:
- Astrophysical Journal Letters, Journal Name: Astrophysical Journal Letters Journal Issue: 2 Vol. 791; ISSN 2041-8205
- Country of Publication:
- United States
- Language:
- English
Similar Records
DISCOVERY OF Hα EMISSION FROM THE CLOSE COMPANION INSIDE THE GAP OF TRANSITIONAL DISK HD 142527
PEERING INTO THE GIANT-PLANET-FORMING REGION OF THE TW HYDRAE DISK WITH THE GEMINI PLANET IMAGER
THE DYNAMICALLY DISRUPTED GAP IN HD 142527
Journal Article
·
Fri Jan 31 23:00:00 EST 2014
· Astrophysical Journal Letters
·
OSTI ID:22364014
PEERING INTO THE GIANT-PLANET-FORMING REGION OF THE TW HYDRAE DISK WITH THE GEMINI PLANET IMAGER
Journal Article
·
Sat Dec 19 23:00:00 EST 2015
· Astrophysical Journal Letters
·
OSTI ID:22518652
THE DYNAMICALLY DISRUPTED GAP IN HD 142527
Journal Article
·
Wed Aug 01 00:00:00 EDT 2012
· Astrophysical Journal Letters
·
OSTI ID:22047641