dc.creator |
Majaess, Daniel J. |
|
dc.creator |
Turner, David Gerald, 1945- |
|
dc.creator |
Gieren, W. |
|
dc.date.accessioned |
2018-04-17T19:05:43Z |
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dc.date.available |
2018-04-17T19:05:43Z |
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dc.date.issued |
2012-04 |
|
dc.identifier.issn |
0035-8711 |
|
dc.identifier.uri |
http://library2.smu.ca/handle/01/27425 |
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dc.description |
Publisher's Version/PDF |
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dc.description.abstract |
Preliminary constraints are placed on a cluster of young stellar objects (J2000 02:54:31.4 +69:20:32.5) discovered in the field of the classical Cepheid SU Cas. The Wide-field Infrared Survey Explorer (WISE) 3.4-, 4.6-, 12- and 22-µm images reveal that the cluster deviates from spherical symmetry and exhibits an apparent diameter of 3 × 6 arcmin. Spectral energy distributions constructed using the Two Micron All Sky Survey (2MASS) K<sub>s</sub> (2.2 µm) and WISE photometry indicate that 19 (36 per cent) class I, 21 (40 per cent) class f and 13 (25 per cent) class II objects lie r < 3 arcmin from the cluster centre. Conversely, 11 (18 per cent) class I, 13 (21 per cent) class f and 37 (61 per cent) class II objects were detected for r > 3 arcmin. Approximately 50 per cent of the class I sources within r < 3 arcmin were classified solely using WISE photometry owing to the absence of detections by 2MASS. |
en_CA |
dc.description.provenance |
Submitted by Betty McEachern (betty.mceachern@smu.ca) on 2018-04-17T19:05:43Z
No. of bitstreams: 1
Majaess_D_article_2012_d.pdf: 473382 bytes, checksum: ae5d43fe677ba2c3a5e717913835e6f8 (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2018-04-17T19:05:43Z (GMT). No. of bitstreams: 1
Majaess_D_article_2012_d.pdf: 473382 bytes, checksum: ae5d43fe677ba2c3a5e717913835e6f8 (MD5)
Previous issue date: 2012-04 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
Oxford Academic |
en_CA |
dc.relation.uri |
https://dx.doi.org/10.1111/j.1365-2966.2011.20366.x |
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dc.rights |
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2012 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. |
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dc.subject.lcsh |
Stars -- Clusters |
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dc.subject.lcsh |
Stars -- Formation |
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dc.subject.lcsh |
Spectral energy distribution |
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dc.subject.lcsh |
Astronomical photometry |
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dc.subject.lcsh |
Infrared astronomy |
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dc.title |
A cluster of class I/f/II young stellar objects discovered near the Cepheid SU Cas |
en_CA |
dc.type |
Text |
en_CA |
dcterms.bibliographicCitation |
Monthly Notices of the Royal Astronomical Society 421(2), 1040-1042. (2012) |
en_CA |