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相关论文: VLT K-band spectroscopy of massive young stellar o…

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High-quality K-band spectra of point sources, deeply embedded in massive star-forming regions, have revealed a population of 20 young massive stars showing no photospheric absorption lines, but only emission lines. The K-band spectra…

天体物理学 · 物理学 2009-11-11 Arjan Bik , Lex Kaper , Wing-Fai Thi , Rens Waters

We have obtained high resolution (R = 10,000) K-band spectra of candidate young massive stars deeply embedded in high-mass star-forming regions. These objects were selected from a near-infrared survey of 44 regions of high-mass…

天体物理学 · 物理学 2007-05-23 A. Bik , L. Kaper , M. M. Hanson , L. B. F. M. Waters

We have obtained high resolution (R = 10,000) K-band spectra of candidate young massive stars deeply embedded in (ultra-) compact HII regions (UCHIIs). In these clusters, three types of objects are identified. The first type (38 objects)…

天体物理学 · 物理学 2009-11-11 A. Bik , L. Kaper , M. M. Hanson , M. Smits

High resolution (lambda / Delta-lambda = 50,000) K-band spectra of massive, embedded, young stellar objects are presented. The present sample consists of four massive young stars located in nascent clusters powering Galactic giant H II…

天体物理学 · 物理学 2009-11-10 R. D. Blum , C. L. Barbosa , A. Damineli , P. S. Conti , S. Ridgway

We present medium-resolution (R $\sim$ 4000) YJ, H \& K band spectroscopy of candidate young stellar objects (YSOs) in NGC~346, the most active star-formation region in the metal-poor (Z = 1/5 Z$_{\sun}$) Small Magellanic Cloud. The spectra…

太阳与恒星天体物理 · 物理学 2022-09-14 O. C. Jones , M. Reiter , R. Sanchez-Janssen , C. J. Evans , C. S. Robertson , M. Meixner , B. Ochsendorf

We present observations of CO overtone bandhead emission toward four massive Young Stellar Objects (spectral type O6--B5). The high signal-to-noise ratio K-band spectra were obtained with VLT-ISAAC at a resolution of 30 km/s, sufficient to…

天体物理学 · 物理学 2016-08-30 A. Bik , W-. F. Thi

Aims: We test the technique of spectro-astrometry as a potential method to investigate the close environment of massive young stars. Method: Archival VLT near infrared K band spectra (R=8900) of three massive young stellar objects and one…

天体物理学 · 物理学 2009-11-11 J. M. C. Grave , M. S. N. Kumar

We have performed intermediate resolution (R = 5000), high signal-to-noise H-band spectroscopy of a small, initial sample of three massive embedded young stellar objects (YSOs), using VLT/ISAAC. The sample has been selected from sources…

天体物理学 · 物理学 2016-08-30 T. R. Kendall , W. J. de Wit , J. L. Yun

We report on the observation of hot water vapor (steam) in the inner AU of a young massive star located in the star-forming region IRAS 08576-4334. The water lines are detected in a medium resolution (R=10,000) K-band spectrum taken by the…

天体物理学 · 物理学 2009-11-10 W. -F. Thi , A. Bik

We present $K$-band integral field spectroscopic observations towards 17 massive young stellar objects (YSOs) in the low metallicity Small Magellanic Cloud (SMC) and two YSO candidates in the compact H ii regions N81 and N88 A (also in the…

星系天体物理 · 物理学 2016-09-21 J. L. Ward , J. M. Oliveira , J. Th. van Loon , M. Sewiło

We present near-IR SINFONI observations of three Galactic HII regions: RVW79, RCW82 and RCW120. We identify the ionizing stars of each region: they are early to late O stars, close to the main sequence. We derive their stellar and wind…

太阳与恒星天体物理 · 物理学 2015-05-14 F. Martins , M. Pomares , L. Deharveng , A. Zavagno , J. -C. Bouret

Near-infrared surveys of high-mass star-forming regions start to shed light onto their stellar content. A particular class of objects found in these regions, the so-called massive Young Stellar Objects (YSOs) are surrounded by dense…

天体物理学 · 物理学 2007-12-04 A. Bik , A. Lenorzer , W-. F. Thi , E. Puga-Antolin , L. B. F. M. Waters , L. Kaper , L. N. Martin-Hernandez

We have carried out a near-infrared imaging survey of luminous young stellar outflow candidates using the United Kingdom Infrared Telescope. Observations were obtained in the broad band K (2.2 mu) and through narrow band filters at the…

太阳与恒星天体物理 · 物理学 2015-05-18 Watson P. Varricatt , Christopher J. Davis , Suzanne Ramsay , Stephen P. Todd

We present Keck Interferometer observations of T Tauri and Herbig Ae/Be stars with a spatial resolution of a few milliarcseconds and a spectral resolution of ~2000. Our observations span the K-band, and include the Br gamma transition of…

太阳与恒星天体物理 · 物理学 2015-06-22 J. A. Eisner , L. A. Hillenbrand , Jordan M. Stone

Massive stars play an important role in many areas of astrophysics, but numerous details regarding their formation remain unclear. In this paper we present and analyse high resolution (R ~ 30,000) near-infrared 2.3 micron spectra of 20…

Circumstellar discs are essential for high mass star formation, while multiplicity, in particular binarity, appears to be an inevitable outcome since the vast majority of massive stars (> 8 Msun) are found in binaries (up to 100%). We…

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 have observed seven ultracompact HII regions in hydrogen recombination lines in the millimeter band. Toward four of these regions, there is a high velocity (full width to half maximum 60-80 km/s) component in the line profiles. The high…

天体物理学 · 物理学 2008-11-26 D. T. Jaffe , J. Martin-Pintado

We present HST/NICMOS observations with 0.1" (15 AU) resolution of six young stellar objects in the Taurus star-formation region. The targets of our survey are three Class I IRAS sources (IRAS 04016+2610, IRAS 04248+2612, and IRAS…

K-band spectra of young stellar candidates in four southern hemisphere clusters have been obtained with the near-infrared spectrograph GNIRS in Gemini South. The clusters are associated with IRAS sources that have colours characteristic of…

天体物理学 · 物理学 2009-11-13 A. Roman-Lopes , Z. Abraham , R. Ortiz , A. Rodrigues-Ardila
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