skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: THE PROTOPLANETARY DISKS IN THE NEARBY MASSIVE STAR-FORMING REGION CYGNUS OB2

Journal Article · · Astrophysical Journal
; ; ; ; ; ;  [1];  [2];  [3]; ;  [4];  [5]
  1. Smithsonian Astrophysical Observatory, MS-67, 60 Garden Street, Cambridge, MA 02138 (United States)
  2. School of Physics, Astronomy and Mathematics, University of Hertfordshire, College Lane, Hatfield AL10 9AB (United Kingdom)
  3. Five College Astronomy Department, Smith College, Northampton, MA 01063 (United States)
  4. School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL (United Kingdom)
  5. Dpto. de Astrofisica, Universidad de La Laguna, E-38206 La Laguna, Tenerife (Spain)

The formation of stars in massive clusters is one of the main modes of the star formation process. However, the study of massive star-forming regions is hampered by their typically large distances to the Sun. One exception to this is the massive star-forming region Cygnus OB2 in the Cygnus X region, at the distance of {approx}1400 pc. Cygnus OB2 hosts very rich populations of massive and low-mass stars, being the best target in our Galaxy to study the formation of stars, circumstellar disks, and planets in the presence of massive stars. In this paper, we combine a wide and deep set of photometric data, from the r band to 24 {mu}m, in order to select the disk-bearing population of stars in Cygnus OB2 and identify the class I, class II, and stars with transition and pre-transition disks. We selected 1843 sources with infrared excesses in an area of 1 Degree-Sign Multiplication-Sign 1 Degree-Sign centered on Cyg OB2 in several evolutionary stages: 8.4% class I, 13.1% flat-spectrum sources, 72.9% class II, 2.3% pre-transition disks, and 3.3% transition disks. The spatial distribution of these sources shows a central cluster surrounded by an annular overdensity and some clumps of recent star formation in the outer region. Several candidate subclusters are identified, both along the overdensity and in the rest of the association.

OSTI ID:
22130988
Journal Information:
Astrophysical Journal, Vol. 773, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English

Similar Records

OPTICAL PHOTOMETRIC GTC/OSIRIS OBSERVATIONS OF THE YOUNG MASSIVE ASSOCIATION CYGNUS OB2
Journal Article · Mon Oct 15 00:00:00 EDT 2012 · Astrophysical Journal, Supplement Series · OSTI ID:22130988

Subaru Hyper Suprime-Cam Survey of Cygnus OB2 Complex – I. Introduction, photometry, and source catalogue
Journal Article · Mon Sep 27 00:00:00 EDT 2021 · Monthly Notices of the Royal Astronomical Society · OSTI ID:22130988

AN R- AND I-BAND PHOTOMETRIC VARIABILITY SURVEY OF THE CYGNUS OB2 ASSOCIATION
Journal Article · Wed Jun 01 00:00:00 EDT 2011 · Astrophysical Journal, Supplement Series · OSTI ID:22130988