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We report initial results from IRAC observations of four young stellar clusters. These regions are part of a larger Spitzer survey of 31 young stellar groups and clusters within 1 kpc of the Sun. In each of the four clusters, there are…

We present a multiwavelength study of the NGC 281 complex which contains the young cluster IC 1590 at the center, using deep wide-field optical UBVI_c photometry, slitless spectroscopy along with archival data sets in the near-infrared…

星系天体物理 · 物理学 2015-06-04 Saurabh Sharma , A. K. Pandey , J. C. Pandey , N. Chauhan , K. Ogura , D. K. Ojha , J. Borrissova , H. Mito , T. Verdugo , B. C. Bhatt

We present an updated catalog of X-ray point sources in the inner 500$\arcsec$ ($\sim$20 parsec) of the Galactic Center (GC), where the {\it nuclear star cluster} (NSC) stands, based on a total of $\sim$4.5 Ms of {\it Chandra} observations…

高能天体物理现象 · 物理学 2018-04-04 Zhenlin Zhu , Zhiyuan Li , Mark R. Morris

The connection between high-mass stars and young stellar clusters has been well established by near-IR observations showing young massive stars in HII regions surrounded by clusters of lower mass stars. Mm-wave observations show that these…

天体物理学 · 物理学 2007-05-23 A. R. Tieftrunk , S. T. Megeath , S. Thorwirth

We present Spitzer/IRAC photometry on the star-forming HII region N 90, related to the young stellar association NGC 602 in the Small Magellanic Cloud. Our photometry revealed bright mid-infrared sources, which we classify with the use of a…

天体物理学 · 物理学 2010-05-12 Dimitrios A. Gouliermis , Sascha P. Quanz , Thomas Henning

For many years feedback processes generated by OB-stars in molecular clouds, including expanding ionization fronts, stellar winds, or UV-radiation, have been proposed to trigger subsequent star formation. However, hydrodynamic models…

Observational studies of cluster evolution over moderate redshift ranges (to z ~ 1) are a powerful tool for constraining cosmological parameters, yet a comprehensive knowledge of the properties of these clusters has been hitherto…

天体物理学 · 物理学 2007-05-23 Amalia Hicks , Erica Ellingson , Mark Bautz , Howard Yee , Mike Gladders , Gordon Garmire

The X-ray source populations within galaxies are typically difficult to identify and classify from X-ray data alone. We are able to break through this barrier by combining deep new Chandra ACIS-I observations with extensive Hubble Space…

About 1000 X-ray emitting young pre-main sequence (PMS) stars distributed in mass from 0.05 to 50 solar masses are detected in an image of the Orion Nebula obtained with the Advanced CCD Imaging Spectrometer on board the Chandra X-ray…

We present new optical spectroscopy with FLAMES/VLT, near-IR imaging with HAWK-I/VLT, and 870 micron mapping with APEX/LABOCA of the Coronet cluster. The optical data allow to estimate spectral types, extinction and the presence of…

太阳与恒星天体物理 · 物理学 2015-05-28 Aurora Sicilia-Aguilar , Thomas Henning , Jouni Kainulainen , Veronica Roccatagliata

We present a general method for identifying the pre-main-sequence population of any star-forming region, unbiased with respect to the presence or absence of disks, in contrast to samples selected primarily via their mid-infrared emission…

星系天体物理 · 物理学 2012-08-27 Mary Barsony , Karl E. Haisch, , Kenneth A. Marsh , Chris McCarthy

We offer to the star formation community the third installment of the Massive Star-forming Regions (MSFRs) Omnibus X-ray Catalog (MOXC3), a compilation of X-ray point sources detected in 50 archival Chandra/ACIS observations of 14 Galactic…

高能天体物理现象 · 物理学 2019-10-09 Leisa K. Townsley , Patrick S. Broos , Gordon P. Garmire , Matthew S. Povich

The Massive Young Star Forming Complex in Infrared and X-ray (MYStIX) project provides a new census on stellar members of massive star forming regions within 4 kpc. Here the MYStIX Infrared Excess catalog (MIRES) and Chandra-based X-ray…

太阳与恒星天体物理 · 物理学 2016-12-21 Gregory Romine , Eric D. Feigelson , Konstantin V. Getman , Michael A. Kuhn , Matthew S. Povich

We have obtained high resolution (<1") deep x-ray images of the globular cluster 47Tucanae (NGC 104) with the Chandra X-ray Observatory to study the population of compact binaries in the high stellar density core. A 70 kilosec exposure of…

天体物理学 · 物理学 2019-08-17 Jonathan E. Grindlay , Craig Heinke , Peter D. Edmonds , Stephen S. Murray

Using deep exposures (~10^5 s) with the ROSAT HRI, we have performed flux-limited surveys for X-ray sources in the vicinity of the Hyades-age open stellar clusters NGC 6633 and IC 4756, detecting 31 and 13 sources respectively. Our primary…

天体物理学 · 物理学 2009-10-31 K. R. Briggs , J. P. Pye , R. D. Jeffries , E. J. Totten

We report on the results of a systematic study of X-ray flares from low-mass young stellar objects, using Chandra observations of the main region of the Rho Oph. From 195 X-ray sources, including class I-III sources and some young brown…

天体物理学 · 物理学 2015-06-24 K. Imanishi , H. Nakajima , M. Tsujimoto , K. Koyama , Y. Tsuboi

We analyze the hierarchical structure in the Rosette Molecular Cloud (RMC) using $^{13}$CO J=1-0 data from the Milky Way Imaging Scroll Painting (MWISP) survey with a non-binary Dendrogram algorithm that allows multiple branches to emerge…

星系天体物理 · 物理学 2025-11-05 Suziye He , Yuehui Ma , Hongchi Wang , Renjie Shen , Miaomiao Zhang , Chong Li , Zhenyi Yue , Xiangyu Ou , Xuepeng Chen

The Canis Major OB1 Association has an intriguing scenario of star formation, especially in the Canis Major R1 (CMa R1) region traditionally assigned to a reflection nebula, but in reality an ionized region. This work is focused on the…

星系天体物理 · 物理学 2018-02-07 T. Santos-Silva , J. Gregorio-Hetem , T. Montmerle , B. Fernandes , B. Stelzer

We present the second installment of the Massive Star-forming Regions (MSFRs) Omnibus X-ray Catalog (MOXC2), a compilation of X-ray point sources detected in Chandra/ACIS observations of 16 Galactic MSFRs and surrounding fields. MOXC2…

We study the properties of the coronae of the low-mass stars in the young (~2-3Myr), nearby (~310pc) open cluster IC348 combining X-ray and optical/infrared data. The four existing Chandra observations of IC348 are merged, thus providing a…

太阳与恒星天体物理 · 物理学 2015-06-03 B. Stelzer , T. Preibisch , F. Alexander , P. Mucciarelli , E. Flaccomio , G. Micela , S. Sciortino