Near-infrared imaging observations of the southern massive star-forming region G333.6-0.2

T. Fujiyoshi; C.H. Smith; T.J.T. Moore; S. Lumsden; D. Aitken; P.F. Roche

doi:10.1111/j.1365-2966.2004.08501.x

Near-infrared imaging observations of the southern massive star-forming region G333.6-0.2

T. Fujiyoshi
, C.H. Smith
, T.J.T. Moore
, S. Lumsden
, D. Aitken
, P.F. Roche

Research output: Contribution to journal › Article › peer-review

11 Citations (Scopus)

Abstract

We present near-infrared broad-band JHK' images of the southern massive star-forming region G333.6−0.2. The slope of the K-luminosity function towards the region (0.24 ± 0.01) is considered to be equivalent to that expected for main-sequence stars in the solar neighbourhood. Point sources with their (H−K) colour greater than 1 are more likely to be located in extended emission and it is suggested that these objects are physically associated with the H ii region.

Original language	English
Pages (from-to)	801-809
Journal	Monthly Notices of the Royal Astronomical Society (MNRAS)
Volume	356
Issue number	3
DOIs	https://doi.org/10.1111/j.1365-2966.2004.08501.x
Publication status	Published - 2005

Access to Document

10.1111/j.1365-2966.2004.08501.x

Cite this

@article{fd4384403a8348118a4a31df61bdf677,

title = "Near-infrared imaging observations of the southern massive star-forming region G333.6-0.2",

abstract = "We present near-infrared broad-band JHK' images of the southern massive star-forming region G333.6−0.2. The slope of the K-luminosity function towards the region (0.24 ± 0.01) is considered to be equivalent to that expected for main-sequence stars in the solar neighbourhood. Point sources with their (H−K) colour greater than 1 are more likely to be located in extended emission and it is suggested that these objects are physically associated with the H ii region.",

author = "T. Fujiyoshi and C.H. Smith and T.J.T. Moore and S. Lumsden and D. Aitken and P.F. Roche",

note = "{\textquoteleft}The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing. DOI: 10.1111/j.1365-2966.2004.08501.x [Full text of this article is not available in the UHRA]",

year = "2005",

doi = "10.1111/j.1365-2966.2004.08501.x",

language = "English",

volume = "356",

pages = "801--809",

journal = "Monthly Notices of the Royal Astronomical Society (MNRAS)",

issn = "0035-8711",

publisher = "Oxford University Press (OUP)",

number = "3",

}

TY - JOUR

T1 - Near-infrared imaging observations of the southern massive star-forming region G333.6-0.2

AU - Fujiyoshi, T.

AU - Smith, C.H.

AU - Moore, T.J.T.

AU - Lumsden, S.

AU - Aitken, D.

AU - Roche, P.F.

N1 - ‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing. DOI: 10.1111/j.1365-2966.2004.08501.x [Full text of this article is not available in the UHRA]

PY - 2005

Y1 - 2005

N2 - We present near-infrared broad-band JHK' images of the southern massive star-forming region G333.6−0.2. The slope of the K-luminosity function towards the region (0.24 ± 0.01) is considered to be equivalent to that expected for main-sequence stars in the solar neighbourhood. Point sources with their (H−K) colour greater than 1 are more likely to be located in extended emission and it is suggested that these objects are physically associated with the H ii region.

AB - We present near-infrared broad-band JHK' images of the southern massive star-forming region G333.6−0.2. The slope of the K-luminosity function towards the region (0.24 ± 0.01) is considered to be equivalent to that expected for main-sequence stars in the solar neighbourhood. Point sources with their (H−K) colour greater than 1 are more likely to be located in extended emission and it is suggested that these objects are physically associated with the H ii region.

U2 - 10.1111/j.1365-2966.2004.08501.x

DO - 10.1111/j.1365-2966.2004.08501.x

M3 - Article

SN - 0035-8711

VL - 356

SP - 801

EP - 809

JO - Monthly Notices of the Royal Astronomical Society (MNRAS)

JF - Monthly Notices of the Royal Astronomical Society (MNRAS)

IS - 3

ER -

Near-infrared imaging observations of the southern massive star-forming region G333.6-0.2

Abstract

Access to Document

Fingerprint

Cite this