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Early Planet Formation in Embedded Disks (eDisk). X. Compact Disks, Extended Infall, and a Fossil Outburst in the Class I Oph IRS43 Binary.
- Source :
- Astrophysical Journal; 11/20/2023, Vol. 958 Issue 1, p1-10, 10p
- Publication Year :
- 2023
-
Abstract
- We present the first results from the Early Planet Formation in Embedded Disks Atacama Large Millimeter/submillimeter Array Large Program toward Oph IRS43, a binary system of solar mass protostars. The 1.3 mm dust continuum observations resolve a compact disk, ∼6 au radius, around the northern component and show that the disk around the southern component is even smaller, ≲3 au. CO, <superscript>13</superscript>CO, and C<superscript>18</superscript>O maps reveal a large cavity in a low-mass envelope that shows kinematic signatures of rotation and infall extending out to ∼2000 au. An expanding CO bubble centered on the extrapolated location of the source ∼130 yr ago suggests a recent outburst. Despite the small size of the disks, the overall picture is of a remarkably large and dynamically active region. [ABSTRACT FROM AUTHOR]
- Subjects :
- COMPACT discs
ORIGIN of planets
BINARY stars
PROTOSTARS
FOSSILS
Subjects
Details
- Language :
- English
- ISSN :
- 0004637X
- Volume :
- 958
- Issue :
- 1
- Database :
- Complementary Index
- Journal :
- Astrophysical Journal
- Publication Type :
- Academic Journal
- Accession number :
- 173494323
- Full Text :
- https://doi.org/10.3847/1538-4357/acfd24