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Context. V2492 Cyg is a young eruptive star that went into outburst in 2010. The near-infrared color changes observed since the outburst peak suggest that the source belongs to a newly defined sub-class of young eruptive stars, where…

Young double star V1318 Cyg, which is associated with a small isolated star-forming region around HAeBe star BD+40o4124, has very unusual photometric and spectral behavior. We present results of photometric and spectroscopic observations in…

太阳与恒星天体物理 · 物理学 2019-05-01 T. Yu. Magakian , T. A. Movsessian , H. R. Andreasyan , M. H. Gevorgyan

The variability of Young Stellar Objects (YSOs) is a crucial tool for understanding the mechanisms driving flux changes. In this study, we present an infrared variability analysis of a large sample of over 20,000 candidate YSOs, using data…

太阳与恒星天体物理 · 物理学 2025-03-19 Neha S. , Saurabh

We present $K$-band integral field spectroscopic observations towards 17 massive young stellar objects (YSOs) in the low metallicity Small Magellanic Cloud (SMC) and two YSO candidates in the compact H ii regions N81 and N88 A (also in the…

星系天体物理 · 物理学 2016-09-21 J. L. Ward , J. M. Oliveira , J. Th. van Loon , M. Sewiło

Using the Space Telescope Imaging Spectrograph, we have obtained ultraviolet (UV) spectra from $\sim 1200$ to 2000 \AA\ of known Lyman continuum (LyC) emitting galaxies at low redshift ($z \sim 0.3-0.4$) with varying absolute LyC escape…

星系天体物理 · 物理学 2022-03-02 D. Schaerer , Y. I. Izotov , G. Worseck , D. Berg , J. Chisholm , A. Jaskot , K. Nakajima , S. Ravindranath , T. X. Thuan , A. Verhamme

We present VLBI observations of the H$_2$O maser emission towards a selection of massive young stellar objects (YSOs). In one of these sources, IRAS20126+4104, the measured proper motions confirm that the water masers spots are tracing the…

天体物理学 · 物理学 2007-05-23 M. J. Rioja , L. Moscadelli , R. Cesaroni

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

Variability is a characteristic feature of young stellar objects (YSOs) and could contribute to the large scatter observed in HR diagrams for star forming regions. For typical YSOs, however, the long-term effects of variability are poorly…

太阳与恒星天体物理 · 物理学 2015-06-03 Aleks Scholz

We present ALMA $^{12}$CO (J=1-0, 3-2 and 6-5), $^{13}$CO (J=1-0) and C$^{18}$O (J=1-0) observations of the local Ultra Luminous Infrared Galaxy, IRAS 13120-5453 (dubbed "The Yo-yo"). The morphologies of the three isotopic species differ,…

星系天体物理 · 物理学 2017-05-10 Kazimierz Sliwa , Christine D. Wilson , Susanne Aalto , George C. Privon

We present the combined results of three photometric monitoring campaigns targeting very low mass (VLM) stars and brown dwarfs in the young open cluster IC4665 (age ~40 Myr). In all three runs, we observe ~100 cluster members, allowing us…

太阳与恒星天体物理 · 物理学 2015-05-14 Alexander Scholz , Jochen Eisloeffel , Reinhard Mundt

We present results of continuum and spectral line observations with ALMA and 22 GHz water (H$_2$O) maser observations using KaVA and VERA toward a high-mass star-forming region, G25.82-0.17. Multiple 1.3 mm continuum sources are revealed,…

We have observed the IC1396W globule in a narrow band filter centred on the 1-0 S(1) line of molecular hydrogen and in the J, H, K' broad-band filters. Three molecular hydrogen outflows could be identified by means of H2 emission. The…

天体物理学 · 物理学 2009-11-07 D. Froebrich , A. Scholz

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

V2492 Cyg is a young pre-main sequence star presenting repetitive brightness variations of significant amplitude (Delta R > 5 mag) whose physical origin has been ascribed to both extinction (UXor-type) and accretion (EXor-type) variability,…

太阳与恒星天体物理 · 物理学 2018-04-11 T. Giannini , U. Munari , S. Antoniucci , D. Lorenzetti , A. A. Arkharov , S. Dallaporta , A. Rossi , G. Traven

It has been suggested that IC4499 is one of the very few old globulars to not host multiple populations with light-element variations. To follow-up on this very interesting result, here we make use of accurate HST photometry and FLAMES@VLT…

太阳与恒星天体物理 · 物理学 2018-10-24 E. Dalessandro , C. Lardo , M. Cadelano , S. Saracino , N. Bastian , A. Mucciarelli , M. Salaris , P. Stetson , E. Pancino

Recent studies have identified several young stellar objects (YSOs) which exhibit significant mid-infrared (mid-IR) variability. A wide range of physical mechanisms may be responsible for these variations, including changes in a YSO's…

The HOYS citizen science project conducts long term, multifilter, high cadence monitoring of large YSO samples with a wide variety of professional and amateur telescopes. We present the analysis of the light curve of V1490Cyg in the Pelican…

Far infrared fine structure line data from the ISO archive have been extracted for several hundred YSOs and their outflows, including molecular (CO) outflows, optical jets and Herbig-Haro (HH) objects. Given the importance of these lines to…

天体物理学 · 物理学 2009-11-11 R. Liseau , K. Justtanont , A. G. G. M. Tielens

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

Context. This is the third of a series of papers devoted to study in detail and with high-angular resolution intermediate-mass molecular outflows and their powering sources. Aims. The aim of this paper is to study the intermediate-mass YSO…

天体物理学 · 物理学 2009-11-13 M. T. Beltran , R. Estalella , J. M. Girart , P. T. P. Ho , G. Anglada