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Table · dataset · 2011

Young (proto)stellar population in L1630

Listed in IVOA Registry (Virtual Observatory)

We investigate the young (proto)stellar population in NGC 2023 and the L 1630 molecular cloud bordering the H II region IC 434, using Spitzer IRAC and MIPS archive data, JCMT SCUBA imaging and spectroscopy as well as targeted BIMA observations of one of the Class 0 protostars, NGC 2023 MM 1.

Description

We study the distribution of gas, dust and young stars in this region to see where stars are forming, whether the expansion of the H II region has triggered star formation, and whether dense cold cores have already formed stars.

We have performed photometry of all IRAC and MIPS images, and used color-color diagrams to identify and classify all young stars seen within a 22'x26' field along the boundary between IC 434 and L 1630.

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Stated by source
Infrared
Inferred from text
Image 65% · Imaging 75% · Stellar astronomy and planetary systems 78%
Provenance · 1 source records, 11 field assertions
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