中文
相关论文

相关论文: Spitzer-MIPS Observations of the eta Cha Young Ass…

200 篇论文

We report on mid-infrared imaging observations of the anomalous X-ray pulsars (AXPs) 1E 1048.1-5937, 1RXS J170849-400910, and XTE J1810-197. The observations were carried out at 4.5 and 8.0 microns with the Infrared Array Camera and at 24…

天体物理学 · 物理学 2011-02-11 Z. Wang , V. M. Kaspi , S. J. U. Higdon

We present low-resolution mid-infrared spectra of nine classical T Tauri stars associated with the Chamaeleon I dark cloud. The data were obtained with the PHOT-S instrument on-board the Infrared Space Observatory (ISO) in the two…

天体物理学 · 物理学 2009-10-31 Antonella Natta , Michael R. Meyer , Steven V. W. Beckwith

The disk mass is among the most important input parameter for every planet formation model to determine the number and masses of the planets that can form. We present an ALMA 887micron survey of the disk population around objects from 2 to…

The formation of planets is directly linked to the evolution of the circumstellar (CS) disk from which they are born. The dissipation timescales of CS disks are, therefore, of direct astrophysical importance in evaluating the time available…

We present the results of a multi-wavelength study of circumstellar discs around 44 young stellar objects in the 3 Myr old nearby Chamaeleon I star-forming region. In particular, we explore the far-infrared/submm regime using Herschel…

太阳与恒星天体物理 · 物理学 2015-06-19 Donna Rodgers-Lee , Alexander Scholz , Antonella Natta , Tom Ray

We have performed a search for planetary-mass brown dwarfs in the Chamaeleon I star-forming region using proper motions and photometry measured from optical and infrared images from the Spitzer Space Telescope, the Hubble Space Telescope,…

太阳与恒星天体物理 · 物理学 2017-07-19 T. L. Esplin , K. L. Luhman , J. K. Faherty , E. E. Mamajek , J. J. Bochanski

We have used the Spitzer Space Telescope to obtain Multiband Imaging Photometer for Spitzer (MIPS) 24 um photometry for 37 members of the ~100 Myr old open cluster Blanco 1. For the brightest 25 of these stars (where we have 3sigma…

We describe a search for infra-red excess emission from dusty circumstellar material around 180,000 stars observed by the Kepler and WISE missions. This study is motivated by i) the potential to find bright warm disks around planet host…

地球与行星天体物理 · 物理学 2013-11-07 G. M. Kennedy , M. C. Wyatt

Using the Infrared Array Camera and the Multiband Imaging Photometer aboard the {\it Spitzer Space Telescope}, we have obtained images of the Lupus 3 star-forming cloud at 3.6, 4.5, 5.8, 8.0, and 24 \micron. We present photometry in these…

天体物理学 · 物理学 2008-11-26 P. R. Allen , K. L. Luhman , P. C. Myers , S. T. Megeath , L. E. Allen , L. Hartmann , G. G. Fazio

We present a 1.3 mm continuum survey of the young (2-3 Myr) stellar cluster IC 348, which lies at a distance of 310 pc, and is dominated by low-mass stars (M$_{\star}$ $\sim$ 0.1-0.6 M$_{\odot}$). We observed 136 Class II sources (disks…

We present a Spitzer IRAC and MIPS survey of NGC 2451 A and B, two open clusters in the 50-80 Myr age range. We complement these data with extensive ground-based photometry and spectroscopy to identify the cluster members in the Spitzer…

太阳与恒星天体物理 · 物理学 2011-02-11 Zoltan Balog , Laszlo L. Kiss , Jozsef Vinko , G. H. Rieke , James Muzerolle , Andras Gaspar , Erick T. Young , Nadya Gorlova

We present new deep UBVRI images and high-resolution multi-object optical spectroscopy of the young (~ 6 - 10 Myr old), relatively nearby (800 pc) open cluster IC 2395. We identify nearly 300 cluster members and use the photometry to…

T Cha is a young star surrounded by a transitional disk with signatures of planet formation. We have obtained high-resolution and high-sensitivity ALMA observations of T Cha in the ${\rm CO}(3$--$2)$, ${\rm ^{13}CO}(3$--$2)$, and ${\rm…

太阳与恒星天体物理 · 物理学 2015-02-18 N. Huelamo , I. de Gregorio-Monsalvo , E. Macias , C. Pinte , M. Ireland , P. Tuthill , S. Lacour

Using the MIPS instrument on the Spitzer telescope, we have searched for infrared excesses around a sample of 82 stars, mostly F, G, and K main-sequence field stars, along with a small number of nearby M stars. These stars were selected for…

天体物理学 · 物理学 2008-11-26 C. Beichman , G. Bryden , K. Stapelfeldt

Using the Hubble Space Telescope, the 4 m Blanco telescope at the Cerro Tololo Inter-American Observatory, and the Spitzer Space Telescope, we have performed deep imaging from 0.8 to 8 um of the southern subcluster in the Chamaeleon I…

天体物理学 · 物理学 2009-11-13 K. L. Luhman , Lucia Adame , Paola D'Alessio , Nuria Calvet , Lee Hartmann , S. T. Megeath , G. G. Fazio

We present a large-scale, volume-limited companion survey of 245 late-K to mid-M (K7-M6) dwarfs within 15 pc. Infrared adaptive optics (AO) data were analysed from the Very Large Telescope, Subaru Telescope, Canada-France-Hawaii Telescope,…

太阳与恒星天体物理 · 物理学 2015-06-24 K. Ward-Duong , J. Patience , R. J. De Rosa , J. Bulger , A. Rajan , S. P. Goodwin , Richard J. Parker , D. W. McCarthy , C. Kulesa

We present new Spitzer Space Telescope observations of stars in the young ~5 Myr gamma Velorum stellar cluster. Combining optical and 2MASS photometry, we have selected 579 stars as candidate members of the cluster. With the addition of the…

天体物理学 · 物理学 2009-11-13 Jesus Hernandez , Lee Hartmann , Nuria Calvet , R. D. Jeffries , R. Gutermuth , J. Muzerolle , J. Stauffer

We have conducted a study of debris disks around F stars in order to explore correlations between rotation, stellar winds, and circumstellar disks. We obtained new 24 micron photometry from Spitzer's Multiband Imaging Photometer for Spitzer…

太阳与恒星天体物理 · 物理学 2015-06-11 Trisha Mizusawa , Luisa Rebull , John Stauffer , Geoffrey Bryden , Michael Meyer , Inseok Song

We present low resolution (R = 500) near-infrared spectra of 46 candidate young stellar objects in the Chamaeleon I star-forming region recently detected in several deep photometric surveys of the cloud. Most of these stars have K < 12. In…

天体物理学 · 物理学 2009-11-07 M. Gomez , D. Mardones

T Chamaeleontis is a young star surrounded by a transitional disk, and a plausible candidate for ongoing planet formation. Recently, a substellar companion candidate was reported within the disk gap of this star. However, its existence…

地球与行星天体物理 · 物理学 2017-08-30 A. Cheetham , N. Huelamo , S. Lacour , I. de Gregorio-Monsalvo , P. Tuthill