Masses and Implications for Ages of Low-mass Pre-main-sequence Stars in Taurus and Ophiuchus-Reference-Cited by-同舟云学术

Masses and Implications for Ages of Low-mass Pre-main-sequence Stars in Taurus and Ophiuchus

Published:2019-10-11 Issue:1 Volume:884 Page:42
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Simon M.,Guilloteau S.^ORCID,Beck Tracy L.,Chapillon E.,Folco E. Di,Dutrey A.,Feiden Gregory A.^ORCID,Grosso N.,Piétu V.,Prato L.,Schaefer Gail H.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab3e3b/pdf

Reference53 articles.

1. Submillimeter Observations of the Young Low‐Mass Object IRAS 04158+2805

2. THE MASS DEPENDENCE BETWEEN PROTOPLANETARY DISKS AND THEIR STELLAR HOSTS

3. The Dynamical Complexity of Surface Mass Shedding from a Top-shaped Asteroid Near the Critical Spin Limit

4. New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit

5. Pre-main-sequence isochrones – II. Revising star and planet formation time-scales

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