Pfalzner, Susanne ORCID: 0000-0002-5003-4714, Dehghani, Shahrzad and Michel, Arnaud ORCID: 0000-0003-4099-9026 (2022). Most Planets Might Have More than 5 Myr of Time to Form. Astrophys. J. Lett., 939 (1). BRISTOL: IOP Publishing Ltd. ISSN 2041-8213

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Abstract

The lifetime of protoplanetary disks is a crucial parameter for planet formation research. Observations of disk fractions in star clusters imply median disk lifetimes of 1-3 Myr. This very short disk lifetime calls for planet formation to occur extremely rapidly. We show that young, distant clusters (<= 5 Myr, >200 pc) often dominate these types of studies. Such clusters frequently suffer from limiting magnitudes leading to an over-representation of high-mass stars. As high-mass stars disperse their disks earlier, the derived disk lifetimes apply best to high-mass stars rather than low-mass stars. Including only nearby clusters (<200 pc) minimizes the effect of limiting magnitude. In this case, the median disk lifetime of low-mass stars is with 5-10 Myr, thus much longer than often claimed. The longer timescales provide planets ample time to form. How high-mass stars form planets so much faster than low-mass stars is the next grand challenges.

Item Type: Journal Article
Creators:
CreatorsEmailORCIDORCID Put Code
Pfalzner, SusanneUNSPECIFIEDorcid.org/0000-0002-5003-4714UNSPECIFIED
Dehghani, ShahrzadUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Michel, ArnaudUNSPECIFIEDorcid.org/0000-0003-4099-9026UNSPECIFIED
URN: urn:nbn:de:hbz:38-681165
DOI: 10.3847/2041-8213/ac9839
Journal or Publication Title: Astrophys. J. Lett.
Volume: 939
Number: 1
Date: 2022
Publisher: IOP Publishing Ltd
Place of Publication: BRISTOL
ISSN: 2041-8213
Language: English
Faculty: Unspecified
Divisions: Unspecified
Subjects: no entry
Uncontrolled Keywords:
KeywordsLanguage
YOUNG CLUSTER; SPITZER VIEW; EVOLUTION; DISKS; DISCS; DIVERSITY; ACCRETION; LIFETIMES; DENSITY; STARSMultiple languages
Astronomy & AstrophysicsMultiple languages
URI: http://kups.ub.uni-koeln.de/id/eprint/68116

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