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相关论文: Optical Mass Flow Diagnostics in Herbig Ae/Be Star…

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Herbig Ae/Be objects are pre-main sequence stars surrounded by gas- and dust-rich circumstellar discs. These objects are in the throes of star and planet formation, and their characterisation informs us of the processes and outcomes of…

太阳与恒星天体物理 · 物理学 2016-01-20 N. Pascual , B. Montesinos , G. Meeus , J. P. Marshall , I. Mendigutía , G. Sandell

The large body of near infrared observations presented in Testi et al. (1997; 1998) are analysed with the aim of characterizing the young stellar clusters surrounding Herbig Ae/Be stars. The results confirm the tendency of early Be stars to…

天体物理学 · 物理学 2007-05-23 L. Testi , F. Palla , A. Natta

We use Gaia Data Release 2 (DR2) to place 252 Herbig Ae/Be stars in the HR diagram and investigate their characteristics and properties. For all known Herbig Ae/Be stars with parallaxes in Gaia DR2, we collected their atmospheric parameters…

太阳与恒星天体物理 · 物理学 2018-12-12 M. Vioque , R. D. Oudmaijer , D. Baines , I. Mendigutía , R. Pérez-Martínez

We have observed P-Cygni and asymmetric, blue-shifted absorption profiles in the He I 10830 lines of twelve R Coronae Borealis (RCB) stars over short (1 month) and long (3 year) timescales to look for variations linked to their…

太阳与恒星天体物理 · 物理学 2019-08-19 Geoffrey C. Clayton , T. R. Geballe , Wanshu Zhang

Understanding how young stars gain their masses through disk-to-star accretion is of paramount importance in astrophysics. It affects our knowledge about the early stellar evolution, the disk lifetime and dissipation processes, the way the…

太阳与恒星天体物理 · 物理学 2020-05-08 I. Mendigutía

We develop a new diagnostic method to classify galaxies into AGN hosts, star-forming galaxies, and absorption-dominated galaxies by combining the [O III]/Hbeta ratio with rest-frame U-B color. This can be used to robustly select AGNs in…

(Abridged) We use HIFI maps of the 987 GHz H2O 2(02)-1(11) emission to measure the sizes and shapes of 19 high-mass protostellar envelopes. To identify infall, we use HIFI spectra of the optically thin C18O 9-8 and H2O-18 1(11)-0(00) lines.…

星系天体物理 · 物理学 2019-05-29 Floris van der Tak , Russ Shipman , Thierry Jacq , Fabrice Herpin , Jonathan Braine , Friedrich Wyrowski

We present the analysis of FUSE observations of two Herbig AeBe stars known to harbor young circumstellar disks: HD 100546 and HD 163296. In both cases we detect absorption lines from warm and dense H2. The thermalization of the rotational…

The more massive counterparts of T Tauri stars, Herbig Ae/Be stars, are known to vary in a complex way with no variability mechanism clearly identified. We attempt to characterize the optical variability of HD~37806 (MWC 120) on time scales…

太阳与恒星天体物理 · 物理学 2015-05-19 S. M. Rucinski , K. Zwintz , M. Hareter , G. Pojmanski , R. Kuschnig , J. M. Matthews , D. B. Guenther , A. F. J. Moffat , D. Sasselov , W. W. Weiss

We present linear spectropolarimetric data for eight Herbig Be and four Herbig Ae stars at H alpha, H beta and H gamma. Changes in the linear polarisation are detected across all Balmer lines for a large fraction of the observed objects,…

天体物理学 · 物理学 2008-12-18 J. C. Mottram , J. S. Vink , R. D. Oudmaijer , M. Patel

We present a study of optical Fe II emission in 302 AGNs selected from the SDSS. We group the strongest Fe II multiplets into three groups according to the lower term of the transition (b $^4$F, a $^6$S and a $^4$G terms). These correspond…

宇宙学与河外天体物理 · 物理学 2015-05-18 Jelena Kovacevic , Luka C. Popovic , Milan S. Dimitrijevic

We investigate a sample of 6 Herbig Ae/Be stars belonging to the Orion OB1 association, as well as 73 low mass objects, members of the $\sigma$ Orionis cluster, in order to explore the angular momentum evolution at early stages of…

We have obtained 40 high-resolution circular spectropolarimetric measurements of 12 slowly-pulsating B (SPB) stars, 8 Beta Cephei stars and two Be stars with the ESPaDOnS and NARVAL spectropolarimeters. The aim of these observations is to…

太阳与恒星天体物理 · 物理学 2015-05-13 J. Silvester , C. Neiner , H. F. Henrichs , G. A. Wade , V. Petit , E. Alecian , A. -L. Huat , C. Martayan , J. Power , O. Thizy

The HeII (1640 A) line and the resonance doublet of NV (UV1) provide a good diagnostic tool to constrain the excitation mechanism of hot (Te>40,000K) atmospheric/magnetospheric plasmas in T Tauri stars (TTSs). Making use of the data…

太阳与恒星天体物理 · 物理学 2015-06-16 Ana I Gomez de Castro

The rotating magnetic B stars have oblique dipolar magnetic fields and often anomalous helium and metallic compositions. These stars develop co-rotating torus-shaped clouds by channelling winds from their magnetic poles to an anchored…

天体物理学 · 物理学 2009-11-06 Myron A. Smith , Detlef Groote

We discuss wide-field near-IR imaging of the NGC1333, L1448, L1455 and B1 star forming regions in Perseus. The observations have been extracted from a much larger narrow-band imaging survey of the Taurus-Auriga-Perseus complex. These H2…

天体物理学 · 物理学 2009-06-23 C. J. Davis , P. Scholz , P. Lucas , M. D. Smith , A. Adamson

We present the detection of hydrogen fluoride, HF, in two luminous nearby galaxies NGC 253 and NGC 4945 using the Heterodyne Instrument for the Far-Infrared (HIFI) on board the Herschel Space Observatory. The HF line toward NGC 253 has a…

星系天体物理 · 物理学 2014-03-25 R. R. Monje , S. Lord , E. Falgarone , D. C. Lis , D. A. Neufeld , T. G. Phillips , R. Güsten

We present optical spectra of four intermediate mass candidate young stellar objects that have often been classified as Herbig Ae/Be stars. Typical Herbig Ae/Be emission features are not present in the spectra of these stars. Three of them,…

天体物理学 · 物理学 2009-11-07 P. Manoj , G. Maheswar , H. C. Bhatt

We present observations of far-infrared (50-200 micron) OH and H2O emission of the disk around the Herbig Ae star HD 163296 obtained with Herschel/PACS in the context of the DIGIT key program. In addition to strong [OI] emission, a number…

太阳与恒星天体物理 · 物理学 2015-06-05 D. Fedele , S. Bruderer , E. F. van Dishoeck , G. J. Herczeg , N. J. Evans , J. Bouwman , Th. Henning , J. Green

We investigate the properties of $\sim7000$ narrow-band selected galaxies with strong H$\beta+$[OIII] and [OII] nebular emission lines from the High-$z$ Emission Line Survey (HiZELS) between $z \sim 0.8 - 5.0$. Our sample covers a wide…