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相关论文: UYSO 1 - An Extremely Young Massive Stellar Object

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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 found that at least 18 Young Stellar Object candidates invisible at optical and near-infrared wavelengths, as well as ^12CO emission. They are IRAS point sources with FIR colors similar to those of usual YSOs, and the infrared spectral…

天体物理学 · 物理学 2015-06-24 Ikuru Iwata , Shin-ichiro Okumura , Mamoru Saito

Aims. We report the discovery of a strong outburst of the embedded young stellar object (YSO), namely UKIDSS-J185318.36+012454.5, located in the star-forming region associated with IRAS 18507+0121 source and GAL 034.4+00.23 HII region.…

太阳与恒星天体物理 · 物理学 2017-07-05 E. H. Nikoghosyan , N. M. Azatyan , K. G. Khachatryan

The intermediate-mass star-forming core UYSO 1 has previously been found to exhibit intriguing features. While deeply embedded and previously only identified by means of its (sub-)millimeter emission, it drives two powerful, dynamically…

太阳与恒星天体物理 · 物理学 2015-05-18 H. Linz , O. Krause , H. Beuther , Th. Henning , R. Klein , M. Nielbock , B. Stecklum , J. Steinacker , A. Stutz

We use various analytical techniques to study Young Stellar Objects (YSOs) in an area of approximately $10' \times 10'$ in the IRAS 18456-0223 star-forming region. We use archival optical (Gaia DR3) and infrared (2MASS, UKIDSS, Spitzer,…

太阳与恒星天体物理 · 物理学 2026-03-06 Nilesh Pandey , U. S. Kamath

Near-infrared surveys of high-mass star-forming regions start to shed light onto their stellar content. A particular class of objects found in these regions, the so-called massive Young Stellar Objects (YSOs) are surrounded by dense…

天体物理学 · 物理学 2007-12-04 A. Bik , A. Lenorzer , W-. F. Thi , E. Puga-Antolin , L. B. F. M. Waters , L. Kaper , L. N. Martin-Hernandez

(abridged) We study a previously discovered protostellar source that is deeply embedded and drives an energetic molecular outflow. The source, UYSO1, is located close to IRAS 07029-1215 at a distance of ~1 kpc. The multi-wavelength…

Near-infrared photometry and narrow/broad-band imaging of the massive and luminous young stellar object IRAS 05361+3539 are presented. Imaging observations were made at Mt. Abu while the photometric data were taken from the 2MASS. From the…

天体物理学 · 物理学 2007-05-23 A. Chakraborty , D. K. Ojha , B. G. Anandarao , T. N. Rengarajan

Using infrared photometric data extracted from the 2MASS, IRAS and MSX databases, 142 suspected young stellar objects (YSOs) are selected from about 2 million stars in the Camelopardalis segment of the Milky Way limited by Galactic…

天体物理学 · 物理学 2009-06-25 V. Straizys , V. Laugalys

The luminous Young Stellar Object (YSO) IRAS 07422-2001 is studied in the infrared. We discover star forming activity in embedded clusters located in a cloud detected at mid-IR wavelengths in emission. Multiple outflows are discovered from…

太阳与恒星天体物理 · 物理学 2015-06-04 Watson P. Varricatt

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

We present results from our spectroscopic study, using the Infrared Spectrograph (IRS) onboard the Spitzer Space Telescope, designed to identify massive young stellar objects (YSOs) in the Galactic Center (GC). Our sample of 107 YSO…

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 present a complete low-resolution (R~100) near-infrared spectrum of the substellar object GY11, member of the rho-Ophiuchi young association. The object is remarkable because of its low estimated mass and age and because it is associated…

天体物理学 · 物理学 2009-11-07 L. Testi , A. Natta , E. Oliva , F. D'Antona , F. Comeron , C. Baffa , G. Comoretto , S. Gennari

We report the discovery of a mid-infrared outburst in a Young Stellar Object (YSO) with an amplitude close to 8 mag at $\lambda$$\approx$4.6 $\mu$m. WISEA J142238.82-611553.7 is one of 23 highly variable WISE sources discovered in a search…

We are searching for Young Stellar Objects (YSOs) near the boundary between protostars and pre-main sequence objects, what we have termed transitional YSOs. We have identified a sample of 125 objects as candidate transitional YSOs on the…

天体物理学 · 物理学 2007-05-23 A. W. Volp , E. A Magnier , M. E. van den Ancker , L. B. F. M. Waters

Since the '80s the \textit{Einstein} observatory has shown the Young Stellar Objects (YSOs), emit X-rays with luminosities, in the 0.3--8 keV bandpass, up to $\rm 10^3$--$\rm 10^4$ times than the Sun and that the X-ray emission is highly…

太阳与恒星天体物理 · 物理学 2023-04-05 Salvatore Sciortino

Utilizing a decade-long unTimely dataset, supplemented by multi-band data from archives, we search for young stellar objects (YSOs) with variations larger than one magnitude in W1 band within a region of 110 square degrees in the Galactic…

太阳与恒星天体物理 · 物理学 2024-06-27 Jiaxun Li , Tinggui Wang

Young stellar objects (YSOs) may undergo periods of active accretion (outbursts), during which the protostellar accretion rate is temporarily enhanced by a few orders of magnitude. Whether or not these accretion outburst YSOs possess…

This work aims at investigating the molecular and infrared components in the massive young stellar object (MYSO) candidate IRAS 18544+0112. The purpose is to determine the nature and the origin of this infrared source. To analyze the…

星系天体物理 · 物理学 2015-05-14 M. E. Ortega , S. Paron , S. Cichowolski , M. Rubio , G. Castelletti , G. Dubner
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