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相关论文: Star formation toward the H~II region IRAS 10427-6…

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Rich in HII regions, giant molecular clouds are natural laboratories to study massive stars and sequential star formation. The Galactic star forming complex W33 is located at l=~12.8deg and at a distance of 2.4 kpc, has a size of ~10 pc and…

We present observations of an H$\alpha$ emitting knot in the thick disk of NGC 4013, demonstrating it is an H II region surrounding a cluster of young hot stars $z = 860$ pc above the plane of this edge-on spiral galaxy. With LBT/MODS…

We report NIR broad and narrow band photometric observations in the direction of the IRAS17149-3916 source that reveal the presence of a young cluster of massive stars embedded in an HII region coincident with RCW121. These observations,…

天体物理学 · 物理学 2008-11-26 Alexandre Roman-Lopes , Zulema Abraham

We present multi-wavelength analysis around mid-infrared bubble N14 to probe the signature of triggered star formation as well as the formation of new massive star(s) and/or cluster(s) on the borders of the bubble by the expansion of the H…

星系天体物理 · 物理学 2015-06-12 L. K. Dewangan , D. K. Ojha

As part of a systematic study that we are performing with the aim to increase the observational evidence of triggered star formation in the surroundings of HII regions, we analyze the ISM around the HII region G35.673-00.847, a poorly…

星系天体物理 · 物理学 2015-05-20 S. Paron , A. Petriella , M. E. Ortega

We present the radio continuum, infrared, and CO molecular observations of infrared dark cloud (IRDC) G38.95-0.47 and its adjacent H II regions G38.91-0.44 (N74), G38.93-0.39 (N75), and G39.30-1.04. The Purple Mountain Observation (PMO)…

星系天体物理 · 物理学 2015-06-17 Jin-Long Xu , Jun-Jie Wang , Xiao-Lan Liu

We present high-resolution radio continuum observations of the nascent starburst in the metal-poor galaxy SBS 0335-052. These radio data were taken with the Very Large Array and include observations at 0.7cm, 1.3cm, 2cm, 3.6cm, and 6cm.…

宇宙学与河外天体物理 · 物理学 2009-11-13 K. E. Johnson , L. K. Hunt , A. E. Reines

Using photometric data of infrared surveys, young stellar object (YSO) status is verified for 141 objects selected in our previous papers in the Cassiopeia and Camelopardalis segment of the Milky Way bounded by Galactic coordinates (l, b) =…

太阳与恒星天体物理 · 物理学 2018-03-14 V. Straizys , A. Kazlauskas

We report the discovery of a star-forming loop around the young, Crab-like supernova remnant (SNR) G54.1+0.3 using the AKARI infrared satellite. The loop consists of at least eleven young stellar objects (YSOs) embedded in a ring-like…

The region surrounding the well-known reflection nebula, NGC 7023, illuminated by a Herbig Be star, HD 200775, located in the dark cloud L1174 is studied in this work. Based on the distances and proper motion values from Gaia DR2 of 20…

太阳与恒星天体物理 · 物理学 2020-05-04 Piyali Saha , Maheswar G. , Kamath U. S. , Lee C. W , Manoj P. , Blesson Mathew , Ekta Sharma

W4 is a giant H{\sc ii} region ionized by the OB stars of the cluster IC~1805. The H{\sc ii} region/cluster complex has been a subject of numerous investigations as it is an excellent laboratory for studying the feedback effect of massive…

星系天体物理 · 物理学 2017-05-03 Neelam Panwar , M. R. Samal , A. K. Pandey , J. Jose , W. P. Chen , D. K. Ojha , K. Ogura , H. P. Singh , R. K. Yadav

K-band spectra of young stellar candidates in four southern hemisphere clusters have been obtained with the near-infrared spectrograph GNIRS in Gemini South. The clusters are associated with IRAS sources that have colours characteristic of…

天体物理学 · 物理学 2009-11-13 A. Roman-Lopes , Z. Abraham , R. Ortiz , A. Rodrigues-Ardila

The Milky Way contains thousands of H II region candidates identified by their characteristic mid-infrared morphology, but lacking detections of ionized gas tracers such as radio continuum or radio recombination line emission. These targets…

星系天体物理 · 物理学 2021-03-17 William P. Armentrout , Loren D. Anderson , Trey V. Wenger , Dana S. Balser , Thomas M. Bania

The S235A-B star forming region has been extensively observed in the past from the radio to the near-IR, but what was happening in the immediate surroundings of the water maser, placed in between the two nebulosities, was still unclear…

天体物理学 · 物理学 2009-11-10 M. Felli , F. Massi , A. Navarrini , R. Neri , R. Cesaroni , T. Jenness

Chemical abundances in the Leo ring, the largest HI cloud in the local Universe, have recently been determined to be close or above solar, incompatible with a previously claimed primordial origin of the ring. The gas, pre-enriched in a…

星系天体物理 · 物理学 2021-07-21 Edvige Corbelli , Filippo Mannucci , David Thilker , Giovanni Cresci , Giacomo Venturi

Far ultraviolet (FUV) spectral images of the Spica H II region are first presented here for the Si II* 1533.4A and Al II 1670.8A lines and then compared with the optical Halpha image. The H alpha and Si II* images show enhanced emissions in…

太阳与恒星天体物理 · 物理学 2015-05-19 J. -W. Park , K. -W. Min , K. -I. Seon , W. Han , J. Edelstein

IC 417 is in the Galactic Plane, and likely part of the Aur OB2 association; it is ~2 kpc away. Stock 8 is one of the densest cluster constituents; off of it to the East, there is a 'Nebulous Stream' (NS) that is dramatic in the infrared…

Using the ISOPHOT Serendipity Survey (ISOSS) at 170um a sample of galactic star-forming regions exhibiting very cold dust temperatures (< 20 K) and high masses (> 100 M_sun) has been established. We characterise the star-forming content of…

天体物理学 · 物理学 2010-05-19 M. Hennemann , S. M. Birkmann , O. Krause , D. Lemke

IRAS19410+2336 is a young massive star forming region with an intense outflow activity. We present here spatially resolved NIR spectroscopy which allows us to verify whether the H2 emission detected in this object originates from thermal…

天体物理学 · 物理学 2009-11-13 N. L. Martin-Hernandez , A. Bik , E. Puga , D. E. A. Nurnberger , L. Bronfman

We investigated the distributions of classified young stellar object (YSO) in nine star-forming regions associated with Hii regions, namely Sh2-22, Sh2-19, Sh2-17, M16, M8, IC5070, Sh2-252, NGC2467 and M42, as a means of exploring the star…

星系天体物理 · 物理学 2025-11-13 Annarien G. Headley , James O. Chibueze