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相关论文: The Massive Star Forming Region, Cygnus OB2

200 篇论文

Three presumably young eclipsing binary systems in the direction of the Cygnus OB1, OB3 and OB9 associations are studied. Component spectra are reconstructed and their orbits are determined using light curves and spectra disentangling…

太阳与恒星天体物理 · 物理学 2015-06-19 V. Bakis , H. Hensberge , S. Bilir , H. Bakis , F. Yilmaz , E. Kiran , O. Demircan , M. Zejda , Z. Mikulasek

Deep optical photometric data on the NGC 7538 region were collected and combined with archival data sets from $Chandra$, 2MASS and {\it Spitzer} surveys in order to generate a new catalog of young stellar objects (YSOs) including those not…

太阳与恒星天体物理 · 物理学 2017-03-22 Saurabh Sharma , A. K. Pandey , D. K. Ojha , Himali Bhatt , K. Ogura , N. Kobayashi , R. Yadav , J. C. Pandey

We present results of a high angular resolution survey of massive OB stars in the Cygnus OB2 association that we conducted with the NIRI camera and ALTAIR adaptive optics system of the Gemini North telescope. We observed 74 O- and early…

We have investigated the young stellar population in and around SFO 38, one of the massive globules located in the northern part of the Galactic HII region IC 1396, using the Spitzer IRAC and MIPS observations (3.6 to 24 micron) and…

星系天体物理 · 物理学 2015-05-18 Rumpa Choudhury , Bhaswati Mookerjea , H. C. Bhatt

We present the analyses of the stellar contents associated with the HII region Sh2-252 using UBVRI photometry, slit and slitless spectroscopy along with the NIR data from 2MASS for an area ~1 degree x 1 degree. We studied the sub-regions of…

太阳与恒星天体物理 · 物理学 2013-01-01 Jessy Jose , A. K. Pandey , K. Ogura , M. R. Samal , D. K. Ojha , B. C. Bhatt , N. Chauhan , C. Eswaraiah , H. Mito , N. Kobayashi , R. K. Yadav

OB stars are crucial for our understanding of Galactic structure, star formation, stellar feedback and multiplicity. In this paper we have compiled a census of all OB stars within 1 kpc of the Sun. We performed evolutionary and atmospheric…

太阳与恒星天体物理 · 物理学 2025-03-12 Alexis L. Quintana , Nicholas J. Wright , Juan Martínez García

We present mid-infrared (MIR) observations, made with the TIMMI2 camera on the ESO 3.6 m telescope, toward 14 young massive star-forming regions. All regions were imaged in the N band, and nine in the Q band, with an angular resolution of ~…

星系天体物理 · 物理学 2011-02-11 Esteban F. E. Morales , Diego Mardones , Guido Garay , Kate J. Brooks , Jaime E. Pineda

We present deep 1.2 millimeter photometry of 37 stars in the young (5 Myr) Upper Scorpius OB association, sensitive to ~4 x 10^-3 Mjup of cool millimeter dust. Disks around four low- and solar-mass stars are detected, as well as one debris…

太阳与恒星天体物理 · 物理学 2015-06-03 Geoffrey S. Mathews , Jonathan P. Williams , Francois Ménard , Neil Phillips , Gaspard Duchêne , Christophe Pinte

Wide field near-infrared observations and Spitzer Space Telescope IRAC observations of the DR21/W75 star formation regions are presented. The photometric data are used to analyse the extinction, stellar content and clustering in the entire…

天体物理学 · 物理学 2008-11-26 M. S. N. Kumar , C. J. Davis , J. M. C. Grave , B. Ferreira , D. Froebrich

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 detection of 1.809 MeV gamma-ray line emission from the Cygnus X complex by the COMPTEL telescope is one of the most convincing proves of massive star nucleosynthesis in our Galaxy. The Cygnus X complex is an extremely active nearby…

天体物理学 · 物理学 2007-05-23 J. Knodlseder , M. Cervino , D. Schaerer , P. von Ballmoos , G. Meynet

Massive, O and early B-type (OB) stars remain incompletely catalogued in the nearby Galaxy due to high extinction, bright visible and infrared nebular emission in H II regions, and high field star contamination. These difficulties are…

太阳与恒星天体物理 · 物理学 2017-04-19 Matthew S. Povich , Heather A. Busk , Eric D. Feigelson , Leisa K. Townsley , Michael A. Kuhn

Mid-infrared (MIR) shells or bubbles around expanding H II regions have received much attention due to their ability to initiate a new generation of star formation. We present multi-wavelength observations around two bubbles associated with…

星系天体物理 · 物理学 2015-06-05 L. K. Dewangan , D. K. Ojha , B. G. Anandarao , S. K. Ghosh , S. Chakraborti

We present 500 AU and 700 AU resolution 1 mm and 3 mm ALMA observations, respectively, of protostellar cores in protoclusters Sagittarius B2 (Sgr B2) North (N) and Main (M), parts of the most actively star-forming cloud in our Galaxy.…

Studying the stellar populations in the outskirts of spiral galaxies can provide important constraints on their structure, formation, and evolution. To that end, we present VI photometry obtained with the Advanced Camera for Surveys for…

天体物理学 · 物理学 2008-11-26 Michael K. Barker , Ata Sarajedini , Doug Geisler , Paul Harding , Robert Schommer

We present initial results of the first panoramic search for high-amplitude near-infrared variability in the Galactic Plane. We analyse the widely separated two-epoch K-band photometry in the 5th and 7th data releases of the UKIDSS Galactic…

We present the first direct measurement of the spatial cross-correlation function of high-mass X-ray binaries (HMXBs) and active OB star-forming complexes in the Milky Way. This result relied on a sample containing 79 hard X-ray selected…

高能天体物理现象 · 物理学 2012-02-01 Arash Bodaghee , John A. Tomsick , Jerome Rodriguez , J. Berian James

Cygnus OB2 is a rich OB association in the Galaxy which has experienced intense star formation in the last 20-25 Myr. Its stellar population shows a correlation between age and Galactic longitude. Exploring the chemical composition of its…

太阳与恒星天体物理 · 物理学 2018-12-05 S. R. Berlanas , A. Herrero , F. Comerón , S. Simón-Díaz , M. Cerviño , A. Pasquali

Context: The Ara OB1a association is a nearby complex in the fourth Galactic quadrant where a number of young/embedded star clusters are projected close to more evolved, intermediate age clusters. It is also rich in interstellar matter, and…

星系天体物理 · 物理学 2016-08-14 G. Baume , G. Carraro , F. Comeron , G. C. de Elıa

The origins of all extra-solar cosmic rays -- both the ultra high-energy and lower energy Galactic variety -- remain unclear. It has been argued that the large scale shocks and turbulence induced by the multiple interacting supersonic winds…