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相关论文: New Herbig Ae/Be stars confirmed via high-resoluti…

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We report near-infrared photometric measurements of 35 Herbig Ae/Be candidate stars obtained with direct imaging and aperture photometry. Observations were made through the broadband J, H, and K' filters, with each source imaged in at least…

星系天体物理 · 物理学 2015-05-13 Ryan L. Doering , Margaret Meixner

We present optical spectroscopy observations of 145 high-mass pre-main sequence candidates from the catalogue of Vioque et al. (2020). From these, we provide evidence for the Herbig nature of 128 sources. This increases the number of known…

We have carried out a study of the early type stars in nearby OB associations spanning an age range of $\sim$ 3 to 16 Myr, with the aim of determining the fraction of stars which belong to the Herbig Ae/Be class. We studied the B, A, and F…

天体物理学 · 物理学 2009-11-10 Jesus Hernandez , Nuria Calvet , Lee Hartmann , Cesar Briceno , Aurora Sicilia-Aguilar , Perry Berlind , .

Herbig Ae/Be stars (HAeBes) are critical tracers of intermediate- and high-mass star formation, yet their census remains incomplete compared to low-mass young stellar objects like T-Tauri stars. To expand the known population, we…

太阳与恒星天体物理 · 物理学 2026-01-21 Jialin Liu , Jiaming Liu , Jiya Yao , Zhenghao Cheng , Qingyue Qu , Zhicun Liu , Wenyuan Cui , Min Fang

We derive a catalog of early-type emission-line stars including 30,048 spectra of 25,886 stars from LAMOST DR7, in which 3,922 have Simbad records. The sample is obtained using K-Nearest Neighbor and Random Forest methods and visually…

太阳与恒星天体物理 · 物理学 2022-03-30 Yun-Jun Zhang , Wen Hou , A-Li Luo , Shuo Li , Li Qin , Yan Lu , Yin-Bi Li , Jian-Jun Chen , Yong-Heng Zhao

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 present near-IR (J,H,Ks) photometry for 27 of the 28 candidate Herbig Ae/Be stars in the Small and Large Magellanic Clouds identified via the EROS1 and EROS2 surveys as well as near-contemporaneous optical (H-alpha) spectroscopy for 21…

太阳与恒星天体物理 · 物理学 2015-05-28 Bradley W. Rush , John P. Wisniewski , Karen S. Bjorkman

We present VLT-FORS2 optical (5700 - 9400 A) spectroscopy of close (r < 1.5'') companions to three nearby (d < 200 pc) Herbig Ae/Be stars (HD 144432, HD 150193, KK Oph) and one T Tauri star (S CrA). We report the detection of Li I (6707 A)…

天体物理学 · 物理学 2009-11-13 A. Carmona , M. E van den Ancker , Th. Henning

The number of well-studied early-type pre-main-sequence objects is very limited, hampering the study of massive star formation from an observational point of view. Here, we present the results of VLT/FORS2 spectropolarimetric and…

太阳与恒星天体物理 · 物理学 2015-08-06 K. M. Ababakr , J. R. Fairlamb , R. D. Oudmaijer , M. E. van den Ancker

We performed a systematic search for Chandra archival observations of Herbig Ae/Be stars. These stars are fully radiative and not expected to support dynamo action analogous to their convective lower-mass counterparts, the T Tauri stars.…

天体物理学 · 物理学 2009-11-11 B. Stelzer , G. Micela , K. Hamaguchi , J. H. M. M. Schmitt

We present high resolution spectro-astrometry of a sample of 28 Herbig Ae/Be and 3 F-type pre-main sequence stars. The spectro-astrometry is shown from both empirical and simulated data to be capable of detecting binary companions that are…

天体物理学 · 物理学 2009-11-11 Deborah Baines , Rene Oudmaijer , John Porter , Monica Pozzo

We present Halpha linear spectropolarimetry of a large sample of Herbig Ae/Be stars. Together with newly obtained data for 17 objects, the sample contains 56 objects, the largest such sample to date. A change in linear polarization across…

太阳与恒星天体物理 · 物理学 2017-09-20 Karim Ababakr , Rene Oudmaijer , Jorick Vink

We identify 20 F-type Herbig stars and provide a list of 22 pre-main-sequence candidates from LAMOST DR8. The effective temperature, distance, extinction, stellar luminosity, mass, and radius are derived for each Herbig star based on…

太阳与恒星天体物理 · 物理学 2022-09-21 Yun-Jin Zhang , A-Li Luo , Bi-Wei Jiang , Wen Hou , Fang Zuo , Bing Du , Shuo Li , Yong-Heng Zhao

Herbig Ae/Be stars span a key mass range that links low and high mass stars, and thus provide an ideal window from which to explore their formation. This paper presents VLT/X-Shooter spectra of 91 Herbig Ae/Be stars, HAeBes; the largest…

太阳与恒星天体物理 · 物理学 2015-09-09 J. R. Fairlamb , R. D. Oudmaijer , I. Mendigutía , J. D. Ilee , M. E. van den Ancker

Early Herbig Be (HBe) stars are massive, young stars accreting through the Boundary Layer mechanism. However, given the rapid ($<$ 2 Myr) evolution of early Herbig stars to the main-sequence phase, studying the evolution of the…

太阳与恒星天体物理 · 物理学 2023-11-08 B. Shridharan , Blesson Mathew , R. Arun , T. B. Cysil , A. Subramaniam , P. Manoj , G. Maheswar , T. P. Sudheesh

We present high spectral-resolution optical spectra of 49 Herbig Ae/Be stars in a search for the [O I] 6300.2 A line. The vast majority of the stars in our sample show narrow (FWHM < 100 km/s) emission lines, centered on the stellar radial…

天体物理学 · 物理学 2007-05-23 M. E. van den Ancker , B. Acke , C. P. Dullemond

Spectroscopic data are necessary to break degeneracies in asteroseismic modelling of the interior structure in high- and intermediate-mass stars. We derive precise photospheric stellar parameters for a sample of 166 B-type stars with TESS…

The polarization of light across individual spectral lines contains information about the circumstellar environment on very small spatial scales. We have obtained a large number of high precision, high resolution spectropolarimetric…

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

Herbig Ae/Be stars are intermediate-mass pre-main sequence stars undergoing accretion through their circumstellar disk. The optical and infrared (IR) spectra of HAeBe stars show HI emission lines belonging to Balmer, Paschen and Brackett…

太阳与恒星天体物理 · 物理学 2023-06-28 B. Shridharan , Blesson Mathew , R. Arun , T. B. Cysil

Aims: We investigated in detail nine sources in the direction of the young sigma Orionis cluster, which is considered a unique site for studying stellar and substellar formation. The nine sources were selected because of some peculiar…

天体物理学 · 物理学 2009-11-13 J. A. Caballero , L. Valdivielso , E. L. Martin , D. Montes , S. Pascual , P. G. Perez-Gonzalez
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