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相关论文: Herbig Ae/Be Stars in the Magellanic Bridge

200 篇论文

The close environment of four old Pre-Main Sequence stars has been observed thanks to the coronagraphic mode of the HST/NICMOS2 camera at lambda=1.6 micron. In the course of this program, the detection of a circumstellar annulus around HD…

天体物理学 · 物理学 2009-10-31 J. C. Augereau , A. M. Lagrange , D. Mouillet , F. Menard

The LMC star, SSTISAGE1C J050756.44-703453.9, was first noticed during a survey of EROS-2 lightcurves for stars with large irregular brightness variations typical of the R Coronae Borealis (RCB) class. However, the visible spectrum showing…

We present a cluster analysis of the bright main-sequence and faint pre--main-sequence stellar populations of a field ~ 90 x 90 pc centered on the HII region NGC 346/N66 in the Small Magellanic Cloud, from imaging with HST/ACS. We extend…

宇宙学与河外天体物理 · 物理学 2012-08-03 Dimitrios A. Gouliermis , Stefan Schmeja , Volker Ossenkopf , Ralf S. Klessen , Andrew E. Dolphin

Herbig Ae/Be stars lie in the mass range between low and high mass young stars, and therefore offer a unique opportunity to observe any changes in the formation processes that may occur across this boundary. This paper presents medium…

We exploit the first data release from the Gaia mission to identify candidate Mira variables in the outskirts of the Magellanic Clouds. The repeated observations of sources during the initial phase of the Gaia mission is used to identify…

星系天体物理 · 物理学 2017-03-22 Alis J. Deason , Vasily Belokurov , Denis Erkal , Sergey E. Koposov , Dougal Mackey

In order to look for signs of on-going planet formation in young disks, we carried out the first J-band polarized emission imaging of the Herbig Ae/Be stars HD 150193, HD 163296, and HD 169142 using the Gemini Planet Imager (GPI), along…

We quadruple the number of quasars known behind the Large Magellanic Cloud (LMC) from 55 (42 in the LMC fields of the third phase of the Optical Gravitational Lensing Experiment (OGLE)) to 200 by spectroscopically confirming 169 (144 new)…

We report our initial discovery of 73 new planetary nebulae (PNe) in the Large Magellanic Cloud (LMC) following confirmatory 2dF spectroscopy on the Anglo-Australian Telescope (AAT). Preliminary candidate sources come from a 10 per cent…

天体物理学 · 物理学 2009-11-13 Warren A. Reid , Quentin A. Parker

The Magellanic Clouds (MCs) offer an outstanding variety of young stellar associations, in which large samples of low-mass stars (with masses less than 1 solar mass) currently in the act of formation can be resolved and explored…

We present a study of the abundance of Be stars in open clusters as a function of the cluster age, using whenever possible ages determined through Stromgren uvby photometry. For the first time in studies of this kind we have considered…

天体物理学 · 物理学 2007-05-23 Juan Fabregat , J. Miguel Torrejon

We present a spectroscopic study of 150 Classical Be stars in 39 open clusters using medium resolution spectra in the wavelength range 3800 - 9000 \AA. One-third of the sample (48 stars in 18 clusters) has been studied for the first time.…

太阳与恒星天体物理 · 物理学 2011-08-31 Blesson Mathew , Annapurni Subramaniam

We report on observations of the stellar populations in twelve fields spanning the region between the Magellanic Clouds, made with the Mosaic-II camera on the 4-meter telescope at the Cerro-Tololo Inter-American Observatory. The two main…

天体物理学 · 物理学 2008-12-18 Jason Harris

Using the HiVIS spectropolarimeter built for the Haleakala 3.7m AEOS telescope, we have obtained a large number of high precision spectropolarimetrc observations (284) of Herbig AeBe stars collected over 53 nights totaling more than 300…

天体物理学 · 物理学 2009-11-13 D. M. Harrington , J. R. Kuhn

We report on the serendipitous discovery of ~ 500 low-mass candidate PMS stars in the vicinity of the stellar association LH 52 in the Large Magellanic Cloud. We present evidence that the red faint sequence of these stars seen in the CMD of…

天体物理学 · 物理学 2009-11-13 D. Gouliermis , W. Brandner , Th. Henning

The fields of 8 X-ray sources in the Magellanic Clouds believed to be Be/X-ray binaries have been searched for possible Be star counterparts. BVR and H alpha CCD imaging was employed to identify early type emission stars through colour…

天体物理学 · 物理学 2007-05-23 J. B. Stephens , M. J. Coe , D. A. H. Buckley

This is the first in a series of papers in which we describe and report the analysis of a large survey of Herbig Ae/Be stars in circular spectropolarimetry. Using the ESPaDOnS and Narval high-resolution spectropolarimeters at the…

太阳与恒星天体物理 · 物理学 2015-06-12 E. Alecian , G. A. Wade , C. Catala , J. H. Grunhut , J. D. Landstreet , S. Bagnulo , T. Böhm , C. P. Folsom , S. Marsden , I. Waite

(Abridged version) We present the first detailed imaging polarization observations of six SMC and six LMC clusters, known to have large populations of B-type stars which exhibit excess H-alpha emission, to constrain the evolutionary status…

We present Spitzer/IRAC photometry on the star-forming HII region N 90, related to the young stellar association NGC 602 in the Small Magellanic Cloud. Our photometry revealed bright mid-infrared sources, which we classify with the use of a…

天体物理学 · 物理学 2010-05-12 Dimitrios A. Gouliermis , Sascha P. Quanz , Thomas Henning

We present Space Telescope Imaging Spectrograph (STIS) broad band imagery and optical slitless spectroscopy of three young star clusters in the Small Magellanic Cloud (SMC). MA 1796 and MG 2 were previously known as Planetary Nebulae, and…

天体物理学 · 物理学 2009-11-10 Letizia Stanghellini , Eva Villaver , Richard A. Shaw , Max Mutchler

We present Halpha spectropolarimetry observations of a sample of 23 Herbig Ae/Be stars. A change in the linear polarisation across Halpha is detected in a large fraction of the objects, which indicates that the regions around Herbig stars…

天体物理学 · 物理学 2009-11-07 Jorick S. Vink , Janet E. Drew , Tim J. Harries , Rene D. Oudmaijer