The WFCAM multiwavelength Variable Star Catalog(Corrigendum)
نویسندگان
چکیده
منابع مشابه
A Multiwavelength Picture of the Afgl 5142 Star-forming Region
We present molecular line, H 2 O maser, radio continuum and near infrared maps of the bipolar outtow source AFGL 5142. The high resolution of our molecular CO observations enables us to deene the morphology of the large-scale bipolar outtow into a two lobe structure extending for 2 0 on each side of the center. In the perpendicular direction, we nd consistent evidence for a second, more compact...
متن کاملStar formation in M 33 : multiwavelength signatures across the disk
Aims. We use different tracers, such as Hα, ultraviolet (UV), and infrared (IR) emissions at various wavelengths, to study the dust and star-formation (SF) conditions throughout the disk of M 33. Methods. We derive the radial distribution of dust, of the old and young stellar population using Spitzer and GALEX data, complemented by ground-based optical data and available surveys of atomic and m...
متن کاملA multiwavelength picture of the AFGL 5142 star - formingregionTodd
We present molecular line, H 2 O maser, radio continuum and near infrared maps of the bipolar outtow source AFGL 5142. The high resolution of our molecular CO observations enables us to deene the morphology of the large-scale bipolar outtow into a two lobe structure extending for 2 0 on each side of the center. In the perpendicular direction, we nd consistent evidence for a second, more compact...
متن کاملLuminous Red Variable Star
We report photometry and spectroscopy of the evolution of Nova Sagittarii 1994 #1 (V4332 Sagittarii) during outburst. We compare the photometric and spectral evolution of this outburst to known classes of outbursts – including classical novae and outbursts occurring on symbiotic stars – and find this object does not conform to any known class of outburst. The closest match to the behavior of th...
متن کاملThe Multiwavelength Picture of Star Formation in the Very Young Open Cluster NGC 6383
We review the properties of the very young (∼ 2 Myr) open cluster NGC 6383. The cluster is dominated by the massive binary HD 159176 (O7 V + O7 V). The distance to NGC 6383 is consistently found to be 1.3 ± 0.1 kpc and the average reddening is determined to be E(B−V ) = 0.32 ± 0.02. Several pre-main sequence candidates have been identified using different criteria relying on the detection of em...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2015
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361/201423793e