Search Publications

Star Formation and Evolution of Blister-type H II Region Sh2-112
DOI: 10.3847/1538-4357/abc42e Bibcode: 2020ApJ...905...61P

Bhatt, B. C.; Dewangan, L. K.; Ojha, D. K. +4 more

We report the observational findings of the Sh2-112 H II region by using the multiwavelength data analysis ranging from optical to radio wavelengths. This region is powered by the massive O8V-type star BD +45 3216. The surface density distribution and minimum spanning tree analyses of the young stellar object (YSO) candidates in the region reveal …

2020 The Astrophysical Journal
AKARI Gaia 12
Cross-correlation of Far-infrared Background Anisotropies and CMB Lensing from Herschel and Planck Satellites
DOI: 10.3847/1538-4357/abada1 Bibcode: 2020ApJ...901...34C

Gong, Yan; Cooray, Asantha; Chen, Xuelei +3 more

The cosmic infrared background (CIB) anisotropies and cosmic microwave background (CMB) lensing are powerful measurements for exploring cosmological and astrophysical problems. In this work, we measure the autocorrelation power spectrum of the CIB anisotropies in the Herschel-SPIRE HerMES Large Mode Survey (HeLMS) field, and the cross-power spectr…

2020 The Astrophysical Journal
Herschel 12
IRIS Observations of the Low-atmosphere Counterparts of Active Region Outflows
DOI: 10.3847/1538-4357/abba1d Bibcode: 2020ApJ...903...68P

Polito, Vanessa; Testa, Paola; De Pontieu, Bart +2 more

Active region (AR) outflows have been studied in detail since the launch of Hinode/EIS and are believed to provide a possible source of mass and energy to the slow solar wind. In this work, we investigate the lower atmospheric counterpart of AR outflows using observations from the Interface Region Imaging Spectrograph (IRIS). We find that the IRIS…

2020 The Astrophysical Journal
Hinode IRIS 12
Magnetic Reconnection Invoked by Sweeping of the CME-driven Fast-mode Shock
DOI: 10.3847/1538-4357/abc5b2 Bibcode: 2020ApJ...905..150Z

Lin, Jun; Wang, Jingxiu; Zhang, Yuzong +4 more

Coronal waves exist ubiquitously in the solar atmosphere. They are important not only because of their rich physics but also because they are essential candidates for triggering remote magnetic eruptions. However, the latter mechanism has never been directly confirmed. By revisiting the successive eruptions on 2012 March 7, fast-mode shocks are id…

2020 The Astrophysical Journal
SOHO 12
Optical and Infrared Study of the Obscured B[e] Supergiant High-mass X-Ray Binary IGR J16318-4848
DOI: 10.3847/1538-4357/ab881c Bibcode: 2020ApJ...894...86F

Chaty, Sylvain; Fortin, Francis; Sander, Andreas

The supergiant high-mass X-ray binary IGR J16318-4848 was the first source detected by the INTErnational Gamma-Ray Astrophysics Laboratory satellite in 2003 and distinguishes itself by its high intrinsic absorption and B[e] phenomenon. It is the perfect candidate to study both binary interaction and the environment of supergiant B[e] stars. This s…

2020 The Astrophysical Journal
Gaia Herschel 12
A Systematic Study of Galactic Outflows via Fluorescence Emission: Implications for Their Size and Structure
DOI: 10.3847/1538-4357/ab88b4 Bibcode: 2020ApJ...894..149W

Heckman, Timothy M.; Wang, Bingjie; Norman, Colin A. +1 more

Galactic outflows play a major role in the evolution of galaxies, but the underlying physical processes are poorly understood. This is mainly because we have little information about the outflow structure, especially on large scales. In this paper, we probe the structure of galactic outflows in low-z starbursts using a combination of ultraviolet s…

2020 The Astrophysical Journal
eHST 12
New Light on an Old Problem of the Cores of Solar Resonance Lines
DOI: 10.3847/1538-4357/abadf4 Bibcode: 2020ApJ...901...32J

Judge, Philip G.; Leenaarts, Jorrit; Kleint, Lucia +2 more

We reexamine a 50+ yr old problem of deep central reversals predicted for strong solar spectral lines, in contrast to the smaller reversals seen in observations. We examine data and calculations for the resonance lines of H I, Mg II, and Ca II, the self-reversed cores of which form in the upper chromosphere. Based on 3D simulations, as well as dat…

2020 The Astrophysical Journal
IRIS SOHO 12
Unusual Galactic H II Regions at the Intersection of the Central Molecular Zone and the Far Dust Lane
DOI: 10.3847/1538-4357/abadf6 Bibcode: 2020ApJ...901...51A

Heywood, I.; Ginsburg, Adam; Glover, Simon C. O. +7 more

Sgr E is a massive star formation complex found toward the Galactic center that consists of numerous discrete, compact H II regions. It is located at the intersection between the central molecular zone (CMZ) and the far dust lane of the Galactic bar, similar to "hot spots" seen in external galaxies. Compared with other Galactic star formation comp…

2020 The Astrophysical Journal
Herschel 12
Toward Early-type Eclipsing Binaries as Extragalactic Milestones. II. NLTE Spectral Analysis and Stellar Parameters of the Detached O-type System OGLE-LMC-ECL-06782 in the LMC
DOI: 10.3847/1538-4357/ab6bd0 Bibcode: 2020ApJ...890..137T

Kudritzki, Rolf-Peter; Urbaneja, Miguel A.; Gieren, Wolfgang +5 more

We combine the NLTE spectral analysis of the detached O-type eclipsing binary OGLE-LMC-ECL-06782 with the analysis of the radial velocity curve and light curve to measure an independent distance to the Large Magellanic Cloud (LMC). In our spectral analysis we study composite spectra of the system at quadrature and use the information from radial v…

2020 The Astrophysical Journal
Gaia 12
The Three Young Nuclear Super Star Clusters in NGC 5253
DOI: 10.3847/1538-4357/ab8f94 Bibcode: 2020ApJ...896...84S

Smith, Linda J.; Sabbi, Elena; Ryon, Jenna +1 more

The blue compact dwarf galaxy NGC 5253 hosts a very young central starburst. The center contains intense radio thermal emission from a massive ultracompact H II region (or supernebula) and two massive and very young super star clusters (SSCs), which are seen at optical and infrared wavelengths. The spatial correspondence between these three object…

2020 The Astrophysical Journal
Gaia eHST 12