INTERPRETING NEAR-INFRARED HYDROGEN LINE RATIOS IN T TAURI STARS-Reference-Cited by-同舟云学术

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INTERPRETING NEAR-INFRARED HYDROGEN LINE RATIOS IN T TAURI STARS

Published:2013-11-12 Issue:2 Volume:778 Page:148
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Edwards Suzan,Kwan John,Fischer William,Hillenbrand Lynne,Finn Kimberly,Fedorenko Kristina,Feng Wanda

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/778/i=2/a=148/pdf

Reference69 articles.

1. Profiles of Strong Permitted Lines in Classical T Tauri Stars

2. Predicted colors and flux densities of protostars in theHerschelPACS and SPIRE filters

3. POISSON project

4. Observational studies relating to star formation II.

5. Physical Processes in Gaseous Nebulae. III. The Balmer Decrement.

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1. MINDS: Mid-infrared atomic and molecular hydrogen lines in the inner disk around a low-mass star;Astronomy & Astrophysics;2024-07

2. GIARPS High-resolution Observations of T Tauri stars (GHOsT). V. New insights into disk winds from 3 km s-1 resolution spectroscopy;Astronomy & Astrophysics;2023-12-20

3. JWST Peers into the Class I Protostar TMC1A: Atomic Jet and Spatially Resolved Dissociative Shock Region;The Astrophysical Journal Letters;2023-07-01

4. Spectral classification of young stars using conditional invertible neural networks;Astronomy & Astrophysics;2023-06

5. Pre-main-sequence Brackett Emitters in the APOGEE DR17 Catalog: Line Strengths and Physical Properties of Accretion Columns;The Astrophysical Journal;2022-12-30

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