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相关论文: IRAS 22150+6109 - a young B-type star with a large…

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We present a comprehensive study of a low-mass star-forming region,L1251B, at wavelengths from the near-infrared to the millimeter. L1251B, where only one protostar, IRAS 22376+7455, was known previously, is confirmed to be a small group of…

We present results from a study of two luminous IRAS sources thought to be young massive star-forming regions and which have no previously detected radio continuum emission: IRAS 15596-5301 and IRAS 16272-4837. Our study incorporates…

天体物理学 · 物理学 2007-05-23 K. J. Brooks , G. Garay , D. Mardones , R. P. Norris , M. G. Burton

We present a near-infrared spectroscopic and imaging analysis of the star-forming region IRAS 16475-4609, based on TripleSpec/SOAR spectroscopy and NEWFIRM/CTIO imaging, complemented by archival radio and sub-millimeter data. Our…

星系天体物理 · 物理学 2025-06-11 Felipe Navarete , Sean D. Points , Augusto Damineli

We present the detection and characterization of a peculiar low-mass protostar (IRAS 22129+7000) located ~0.4 pc from Ced 201 Photodissociation Region (PDR) and ~0.2 pc from the HH450 jet. The cold circumstellar envelope surrounding the…

天体物理学 · 物理学 2009-11-13 Javier R. Goicoechea , Olivier Berne , Maryvonne Gerin , Christine Joblin , David Teyssier

IRAS 12272-6240 is a complex star forming region with a compact massive dense clump and several associated masers, located at a well-determined distance of $d=9.3$ kpc from the Sun. For this study, we obtained sub-arcsec broad- and…

星系天体物理 · 物理学 2020-06-29 Mauricio Tapia , Paolo Persi , Miguel Roth , Davide Elia

We have observed the massive star forming region, IRAS 18507+0121, at millimeter wavelengths in 3 mm continuum emission and H13CO+(J=1-0) and SiO(v=0, J=2-1) line emission, and at near-infrared wavelengths between 1.2 and 2.1 microns. Two…

天体物理学 · 物理学 2009-11-10 D. S. Shepherd , D. E. A. Nurnberger , L. Bronfman

We report sensitive ATCA radio-continuum observations toward IRAS 15596-5301 and 16272-4837, two luminous objects (> 2x10^4 Lsun) thought to represent massive star-forming regions in early stages of evolution (due to previously undetected…

天体物理学 · 物理学 2011-03-10 Guido Garay , Kate Brooks , Diego Mardones , Ray P. Norris , Michael G. Burton

We present observations of continuum and molecular lines towards the protostar candidates IRAS 21307+5049 and IRAS 22172+5549. Single-dish maps in the 12CO(2--1), C18O(2--1), HCO+(1--0) lines and sub-mm continuum are compared with…

天体物理学 · 物理学 2009-11-10 F. Fontani , R. Cesaroni , L. Testi , S. Molinari , Q. Zhang , J. Brand , C. M. Walmsley

We report an in-depth study of the F8-type star HD 166191, identified in an ongoing survey for stars exhibiting infrared emission above their expected photospheres in the Wide-field Infrared Survey Explorer all-sky catalog. The fractional…

太阳与恒星天体物理 · 物理学 2015-06-16 Adam Schneider , Inseok Song , Carl Melis , Ben Zuckerman , Mike Bessell , Tara Hufford , Sasha Hinkley

While most sources above 10^5Lsun have already formed an Ultracompact HII region (UCHII), this is not necessarily the case for sources of lower luminosity. Characterizing sources in the transition phase, i.e., very luminous objects without…

天体物理学 · 物理学 2009-11-13 H. Beuther , Q. Zhang , T. R. Hunter , T. K. Sridharan , E. A. Bergin

Aims: We have carried out an infrared study of the southern Galactic massive star forming region associated with IRAS 14416-5937. Methods: This star forming region has been mapped simultaneously in two far infrared bands at ~ 150 & 210…

天体物理学 · 物理学 2009-11-11 S. Vig , S. K. Ghosh , D. K. Ojha , R. P. Verma

We present mid IR spectro-photometric imaging of a sample of eight nearby ($D \leq 240$pc) Herbig Ae/Be stars. The spectra are dominated by photospheric emission (HR6000), featureless infrared excess emission (T~Cha), broad silicate…

天体物理学 · 物理学 2007-05-23 R. Siebenmorgen , T. Prusti , A. Natta , Th. Mueller

We present bispectrum speckle interferometry of the massive protostellar object IRAS 23151+5912 in the near-infrared K' band. The reconstructed image shows the diffuse nebulosity north-east of two point-like sources in unprecedented detail.…

天体物理学 · 物理学 2009-11-11 G. Weigelt , H. Beuther , K. -H. Hofmann , M. R. Meyer , Th. Preibisch , D. Schertl , M. D. Smith , E. T. Young

We present an all-sky sample of 984 candidate intermediate-mass Galactic star-forming regions color-selected from the Infrared Astronomical Satellite (IRAS) Point Source Catalog and morphologically classify each object using mid-infrared…

We report the discovery of a young massive stellar cluster embedded in an extended HII region, invisible at optical wavelengths where the extinction is $A_V \approx 28$ magnitudes, associated with the IRAS source 16177-5018. $J, H$ and…

天体物理学 · 物理学 2009-11-10 Alexandre Roman-Lopes , Zulema Abraham , Jacques Raymond Daniel Lepine

IRAS22475+5939 has been well researched by previous astronomers. But we still get some new characteristics about it, using the first observations in lines of CO J=2-1,13CO J=2-1,13CO J=3-2 by the KOSMA 3 m telescope. The mapping of the…

太阳与恒星天体物理 · 物理学 2015-06-04 X. -L. Liu , J. -J. Wang

High angular resolution H2CO line observations have been carried out for the low mass proto-binary star IRAS 16293-2422 using the OVRO millimeter array. Simultaneous continuum observations reveal that the source most probably contains two…

天体物理学 · 物理学 2007-05-23 F. L. Schoeier , J. K. Jorgensen , E. F. van Dishoeck , G. A. Blake

In the course of a comprehensive mm/submm survey of massive star-forming regions, the vicinities of a sample of 47 luminous IRAS sources were closely investigated with SCUBA and IRAM bolometers in order to search for massive protostellar…

天体物理学 · 物理学 2009-11-10 Jan Forbrich , Katharina Schreyer , Bettina Posselt , Randolf Klein , Thomas Henning

We present the results of millimeter and centimeter continuum observations, made with the IRAM 30m telescope and the VLA, toward a sample of 11 luminous IRAS sources classified as high-mass protostellar object candidates. We find 1.2 mm…

天体物理学 · 物理学 2009-11-13 Á. Sánchez-Monge , A. Palau , R. Estalella , M. T. Beltrán , J. M. Girart

Context. The formation and early evolution of high- and intermediate-mass stars towards the main sequence involves the interplay of stars in a clustered and highly complex environment. To obtain a full census of this interaction, the…

太阳与恒星天体物理 · 物理学 2015-05-28 K. M. Maaskant , A. Bik , L. B. F. M. Waters , L. Kaper , Th. Henning , E. Puga , M. Horrobin , J. Kainulainen
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