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相关论文: Disk Evolution in W5: Intermediate Mass Stars at 2…

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We analyze samples of Spitzer Infrared Spectrograph (IRS) spectra of T Tauri stars in the Ophiuchus, Taurus, and Chamaeleon I star-forming regions, whose median ages lie in the <1 to 2 Myr range. The median mid-infrared spectra of objects…

太阳与恒星天体物理 · 物理学 2014-11-20 E. Furlan , D. M. Watson , M. K. McClure , P. Manoj , C. Espaillat , P. D'Alessio , N. Calvet , K. H. Kim , B. A. Sargent , W. J. Forrest , L. Hartmann

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 Spitzer photometric (IRAC and MIPS) and spectroscopic (IRS low resolution) observations for 314 stars in the Formation and Evolution of Planetary Systems (FEPS) Legacy program. These data are used to investigate the properties…

We describe results from a survey for J=3-2 12CO emission from visible stars with an infrared excess. The line is clearly detected in 21 objects, with molecular gas (>10^-3 Jupiter masses) common in targets with infrared excesses >0.01…

天体物理学 · 物理学 2009-11-10 W. R. F. Dent , J. S. Greaves , I. M. Coulson

As early-type stars with a rotation speed close to their critical velocity, Be stars experience an event called the Be phenomenon. The material in their equator is ejected into outside space during the Be phenomenon and forms a…

太阳与恒星天体物理 · 物理学 2024-02-06 Mingjie Jian , Noriyuki Matsunaga , Biwei Jiang , Haibo Yuan , Ruoyi Zhang

We report on a sensitive infrared search for disks around isolated young planetary-mass objects (PMOs) in the NGC1333 cluster, by stacking 70 Spitzer/IRAC frames at 3.6 and 4.5$\,\mu m$. Our co-added images go >2.3 mag deeper than…

太阳与恒星天体物理 · 物理学 2023-04-19 Aleks Scholz , Koraljka Muzic , Ray Jayawardhana , Victor Almendros-Abad , Isaac Wilson

We report high spectral resolution observations of the CO vibrational overtone emission from the young stellar object 1548C27; our observations include both the CO(2-0) and CO(5-3) bandhead regions. These data and similar observations of…

天体物理学 · 物理学 2009-10-28 Joan Najita , John Carr , Al Glassgold , Frank Shu , Alan Tokunaga

Spitzer Space Observatory IRAC and MIPS photometric observations are presented for 20 white dwarfs with T < 20,000 K and metal-contaminated photospheres. A warm circumstellar disk is detected at GD 16 and likely at PG 1457-086, while the…

地球与行星天体物理 · 物理学 2011-02-11 J. Farihi , M. Jura , B. Zuckerman

We examine the mid-infrared fluxes and spectral energy distributions for metal-poor stars with iron abundances [Fe/H] $\lesssim-5$, as well as two CEMP-no stars, to eliminate the possibility that their low metallicities are related to the…

太阳与恒星天体物理 · 物理学 2015-06-22 Kim A. Venn , Thomas H. Puzia , Mike Divell , Stephanie Cote , David L. Lambert , Else Starkenburg

MWC 778 is an unusual and little-studied young stellar object located in the IC 2144 nebula. Recent spectroscopy by Herbig and Vacca (2008) suggested the presence of an edge-on circumstellar disk around it. We present near-infrared adaptive…

太阳与恒星天体物理 · 物理学 2009-11-13 Marshall D. Perrin , William D. Vacca , James R. Graham

The recent identification of several groups of young stars within 100 parsecs of the Sun has generated widespread interest. Given their proximity and possible age differences, these systems are ideally suited for detailed studies of star…

Physical models of circumstellar disks surrounding pre-main sequence stars are currently constrained primarily by the spectral energy distribution (SED) of the system. Here we present first results from a survey of nearby Herbig Ae stars…

天体物理学 · 物理学 2009-11-07 Philip M. Hinz , William F. Hoffmann , Joseph L. Hora

We look for trends relating the mass accretion rate (Macc) and the stellar ages (t), spectral energy distributions (SEDs), and disk masses (Mdisk) for a sample of 38 HAeBe stars, comparing them to analogous correlations found for classical…

太阳与恒星天体物理 · 物理学 2012-05-23 I. Mendigutía , A. Mora , B. Montesinos , C. Eiroa , G. Meeus , B. Merín , R. D. Oudmaijer

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

We analyze Spitzer IRS spectra of 110 B-, A-, F-, and G-type stars with optically thin infrared excess in the Scorpius-Centaurus (ScoCen) OB association. The age of these stars ranges from 11-17 Myr. We fit the infrared excesses observed in…

地球与行星天体物理 · 物理学 2015-07-24 Hannah Jang-Condell , Christine H. Chen , Tushar Mittal , P. Manoj , Dan Watson , Carey M. Lisse , Erika Nesvold , Marc Kuchner

Disclosing the structure of disks surrounding Herbig AeBe stars is important to expand our understanding of the formation and early evolution of stars and planets. We aim at revealing the sub-AU disk structure around the 10 Myr old Herbig…

太阳与恒星天体物理 · 物理学 2015-05-18 M. Benisty , E. Tatulli , F. Menard , M. Swain

We report on the results of an optical spectroscopic survey designed to confirm the youth and determine the spectral types among a sample of young stellar object (YSO) candidates in the Serpens Molecular Cloud. We observed 150 infrared…

We trace the evolution of eight edge-on star-forming disk galaxies by analyzing stellar population properties of their thin and thick disks. These galaxies have relatively low stellar masses (4~$\times$~10$^9$ to…

We analyze very deep IRAC and MIPS photometry of $\sim$ 12,500 members of the 14 Myr old Double Cluster, h and $\chi$ Persei, building upon on our earlier, shallower Spitzer studies (Currie et al. 2007a, 2008a). Numerous likely members show…

太阳与恒星天体物理 · 物理学 2015-06-22 Ryan Cloutier , Thayne Currie , George Rieke , Scott J. Kenyon , Zoltan Balog , Ray Jayawardhana

We report FUV, optical, and NIR observations of three T Tauri stars in the Orion OB1b subassociation with H$\alpha$ equivalent widths consistent with low or absent accretion and various degrees of excess flux in the mid-infrared. We aim to…