NEAR-ULTRAVIOLET EXCESS IN SLOWLY ACCRETING T TAURI STARS: LIMITS IMPOSED BY CHROMOSPHERIC EMISSION-Reference-Cited by-同舟云学术

NEAR-ULTRAVIOLET EXCESS IN SLOWLY ACCRETING T TAURI STARS: LIMITS IMPOSED BY CHROMOSPHERIC EMISSION

Published:2011-11-29 Issue:2 Volume:743 Page:105
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Ingleby Laura,Calvet Nuria,Bergin Edwin,Herczeg Gregory,Brown Alexander,Alexander Richard,Edwards Suzan,Espaillat Catherine,France Kevin,Gregory Scott G.,Hillenbrand Lynne,Roueff Evelyne,Valenti Jeff,Walter Frederick,Johns-Krull Christopher,Brown Joanna,Linsky Jeffrey,McClure Melissa,Ardila David,Abgrall Hervé,Bethell Thomas,Hussain Gaitee,Yang Hao

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/743/i=2/a=105/pdf

Reference95 articles.

1. Photoevaporation of Circumstellar Disks Due to External Far‐Ultraviolet Radiation in Stellar Aggregates

2. Dust dynamics during protoplanetary disc clearing

3. Photoevaporation of protoplanetary discs – II. Evolutionary models and observable properties

4. A Consistent Model of the Accretion Shock Region in Classical T Tauri Stars

5. Quiescent H2Emission From Pre‐Main‐Sequence Stars in Chamaeleon I

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