ACIS-I observations of NGC 2264. Membership and X-ray properties of PMS stars

2006/04/11 by E. Flaccomio, G. Micela, S. Sciortino · 7 citations
Physics and Astronomy · #Astronomical spectroscopy #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Astrophysics and Star Formation Studies #Galaxy #Hubble sequence #K-type main-sequence star #O-type star #Spectral line #Stars #Stellar classification #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065084

23 pages, 22 figures (one in color), accepted by A&A. (a .pdf file with full resolution versions of figures 1, 2 and 13 is available at http://www.astropa.unipa.it/~ettoref)

arxiv created 2006/04/11 · openalex publication_date 2006/08/04 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims.This paper's goal is to improve the member census of the NGC 2264 star-forming region and study the origin of X-ray activity in young PMS stars.

Citations

• NGC 2264 IRS 1: The Central Engine and Its Cavity
• Chandra Orion Ultradeep Project: Observations and Source Lists
• ChandraX-Ray Observations of Young Clusters. I. NGC 2264 Data
• The Origin of T Tauri X‐Ray Emission: New Insights from the Chandra Orion Ultradeep Project
• A rotational and variability study of a large sample of PMS stars in NGC 2264
• Probing the formation of intermediate- to high-mass stars in protoclusters

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• A Dense Microcluster of Class 0 Protostars in NGC 2264 D-MM1
• Submillimeter array observations of NGC 2264-C: molecular outflows and driving sources
• THE MASSIVE STAR-FORMING REGION CYGNUS OB2. I. CHANDRA CATALOG OF ASSOCIATION MEMBERS