Young Stellar Object Candidates in IC 417 Virtual Observatory Resource

Authors
  1. Rebull et al.
  2. Published by
    NASA/IPAC Infrared Science Archive
Abstract

IC 417 is in the Galactic Plane, and likely part of the Aur OB2 association; it is ~2 kpc away. Stock 8 is one of the densest cluster constituents; off of it to the East, there is a 'Nebulous Stream' (NS) that is dramatic in the infrared (IR). We have assembled a list of literature-identified young stellar objects (YSOs), new candidate YSOs from the NS, and new candidate YSOs from IR excesses. We vetted this list via inspection of the images, spectral energy distributions (SEDs), and color-color/color-magnitude diagrams. We placed the 710 surviving YSOs and candidate YSOs in ranked bins, nearly two-thirds of which have more than 20 points defining their SEDs. The lowest-ranked bins include stars that are confused, or likely carbon stars. There are 503 in the higher-ranked bins; half are SED Class III, and ~40% are SED Class II.

Keywords
  1. survey
See also HTML
https://irsa.ipac.caltech.edu/data/NITARP/IC417/docs/2306.03728.pdf
IVOA Identifier IVOID
ivo://irsa.ipac/NITARP/Catalog/IC417

Access

IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
https://irsa.ipac.caltech.edu/SCS?table=ic417&
IVOA Table Access TAP
https://irsa.ipac.caltech.edu/TAP
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
Web browser access HTML
https://irsa.ipac.caltech.edu/cgi-bin/Gator/nph-dd?catalog=ic417

History

2024-03-14T01:00:00Z
Resource record created
2023-10-16
release

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