C.D.S. - SIMBAD4 rel 1.7 - 2020.11.25CET08:26:24

2015A&A...580A.105P - Astronomy and Astrophysics, volume 580A, 105-105 (2015/8-1)

Sequential planet formation in the HD 100546 protoplanetary disk?


Abstract (from CDS):

The disk around the Herbig Ae star, HD 100546, shows structures that suggest the presence of two companions in the disk at ∼10 and ∼70AU. The outer companion seems to be in the act of formation. Our aims are to provide constraints on the age of the planets in HD 100546 and to explore the potential evidence for sequential planet formation in transition disks such as HD 100546. We compare the recent resolved continuum observations of the disk around HD 100546 with the results of dust evolution simulations using an analytical prescription for the shapes of gaps carved by massive planets. An inner pressure bump must have been present since early in the disk lifetime to have good agreement between the dust evolution models and the continuum observations of HD 100546. This pressure bump may have resulted from the presence of a very massive planet (∼20MJup), which formed early in the inner disk (r∼10AU). If only this single planet exists, the disk is likely to be old, comparable to the stellar age (∼5-10Myr). Another possible explanation is an additional massive planet in the outer disk (r∼70AU): either a low-mass outer planet (≲5MJup) injected at early times, or a higher mass outer planet (> 15MJup) formed very recently, traps the right amount of dust in pressure bumps to reproduce the observations. In the latter case, the disk could be much younger (∼3.0Myr). In the case in which two massive companions are embedded in the disk around HD 100546, as suggested in the literature, the outer companion could be at least >2.5Myr younger than the inner companion.

Abstract Copyright:

Journal keyword(s): protoplanetary disks - circumstellar matter - planet-disk interactions

Simbad objects: 2

goto Full paper

goto View the reference in ADS

Number of rows : 2

N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
1 V* TW Hya TT* 11 01 51.9054298616 -34 42 17.031550898   11.94 10.50 10.626 9.18 K6Ve 1568 1
2 HD 100546 Be* 11 33 25.4404858122 -70 11 41.239343121   6.71 6.30   6.64 A0VaekB8_lB 659 1

    Equat.    Gal    SGal    Ecl

To bookmark this query, right click on this link: simbad:objects in 2015A&A...580A.105P and select 'bookmark this link' or equivalent in the popup menu


© Université de Strasbourg/CNRS

    • Contact