Laurencia is a red algal genus that was described by J.V. Lamouroux in 1813. The main characteristics of this genus have been known as the presence of four pericentral cells in an axial segment, secondary pit connections between adjacent epidermal cells, and the presence of corps en cerise in both epidermal and trichoblast cells. Additionally, the tetrasporangia are arranged in a parallel manner, and male branches feature terminal cup-shaped spermatangial pits. Currently, sixteen Korean Laurencia species have been reported based on their morphological characteristics. In this study, Laurencia decussata and L. pacifica have been added as new records to the Korean algal flora based on a combination of morphological observations and molecular analyses of rbcL sequences. Laurencia decussata has expanded from Australia and New Zealand to Korea, while the distribution of L. pacifica has expanded from USA and Mexico to Korea.

Feldmannia chitonicola is reported as a new record from Korea based on morphological studies in laboratory-cultured materials and molecular analyses. F. chitonicola is mainly characterized by a small size (1-2 mm), erect filaments mostly unbranched, plurilocular sporangia produced on both prostrate and laterally on the basal part of erect filaments, and 2 types (lanceolate and ovate) of sporangia. In our cultures, sporangia production was slower at 10°C than in 16°C and 20°C. Our molecular analyses of rbcL and cox1 genes supported its independence from other congeners reported for Korea. This is the first report of F. chitonicola for western Pacific.

우리는 오리온 분자운 복합체의 북부 필라멘트(이하 NF)에 대하여 12CO (J=1-0) 분자선의 자료를 이용하여 은하 평면이 분자의 운동과 운동학에 미치는 영향을 연구하였다. 6 m 서울대학교 전파망원경(Seoul Radio Astronomy Observatory, SRAO)을 이용하여 2arcmin 공간분해능으로 은하면으로부터 먼 순서로 NF1, NF2, NF3 세 곳을 총 270시간 동안 관측된 자료를 사용하였다. 은하면과 OMC NF는 12CO (J=2-1) 경우 3% 밀도에서, 티끌의 경우 9% 밝기 수준에서 자기장을 따라 서로 연결되어 있었다. 12CO (J=1-0), 12CO (J=2-1), 성간 티끌 관측결과를 비교해본 결과, 세 경우 모두 NF3에서는 고루 분포했지만, NF1과 NF2에서는 비교적 밀도가 높은 특정 영역에서만 함께 나타났다. NF는 단일 구조를 보였으며, NF1에서는 부분 수축 운동을, NF2에서는 하단에서 회전 운동이 나타났고, NF3에서는 유일하게 명확히 자기장에 연관된 나선형 회전이 보였다. 위치-속도 분석 결과, 12CO (J=1-0)를 비롯한 물질들은 NF2와 NF3을 따라 은하면을 향하여 흐를 가능성이 있음을 확인할 수 있었다. 은하면을 향하여 물질이 흐르는 명백한 원인을 이번 연구결과에서 볼 수 없었지만 추후의 더 정교한 관측결과가 NF1과 NF2 상단부의 회전 운동을 확인 할 수 있겠다.

Miridae, commonly plant bugs, is the most diverse group in Heteroptera, with more than 11,000 species, and is widely distributed in the world. This group has a great attention by taxonomists, applied entomologists, and evolutionary biologists because of their great morphological diversity, high biodiversity as well as association with host plants. However, there have been a few phylogenetic studies within this family to date. In this talk, we present the first phylogenetic analyses of the largest tribe Mirini in the family Miridae based on nuclear (18S rRNA and 28S rRNA) and mitochondrial (COI and 16S rRNA) sequence data, based on the results, we discuss on the phylogenetic relationships and classifications within the tribe.

The genus Apolygus China (Hemiptera: Heteroptera: Miridae), comprising 64 species in the world, is one of the most diverse groups in the subfamily Mirinae, including well-known insect pests such as A. spinolae and A. lucorum. A total of 56 species are known in the Palaearctic Region up to date, and most of them have been described from China (28 species), Japan (26 species) and Russia (13 species) respectively. In this talk, taxonomic study on the genus Apolygus from the Korean Peninsula is presented with three Apolygus sp. nov. and two newly recorded species. Photographs and illustrations of diagnostic characters and biological information such as host plants and distributions for each species, and a key to the Korean species are provided. Besides, COI barcoding as a diagnostic tool for this group is discussed emphasizing on the low genetic distances between some species.

The subgenus Nippocallis (Matsumura, 1917) is one of the 10 subgenera of the genus Tuberculatus Mordvilko, 1894. Originally, this subgenus was regarded as an independent genus of the subtribe Myzocallidina by the distinct morphological features and the host plant association with Castanea (Fagaceae). We performed molecular and morphological analyses to determine whether genus Nippocallis belongs to Tuberculatus group. Molecular analysis of the combined data set of Cytochrome Oxidase subunit I COI, Cytochrome B CytB and Elongation Factor I-alpha EF1α indicated that Nippocallis form a sister clade of the genus Myzocallis Passerini, 1860, apart from the genus Tuberculatus. In this contexts, we propose Nippocallis as a separate genus of the subtribe Myzocallidina.

Macrosiphini is the most largest group in aphids, comprising near half of the described aphid species. The existence of Macrosiphini could be related to host alternation and various life cycle. Since the phylogenetic relationship of the tribe Macrosiphini has been still controversial, we analyzed Bayesian phylogeny (BP) and Maximum-likelihood (ML) based on molecular data (cytochrome oxidase I, tRNA-leucine+cytochrome oxidase II, 16S ribosomal RNA and elongation factor-1 alpha gene), and compared with the Shaposhnikov (1998) 's subtribal division: Macrosiphina, Myzian, Anuraphidina and Liosomatinae. Analyses for host range association with the morphological characters (e.g. Siphunculus and antennal tubercle on head) correspond to the tendency of host range radiation in the tribe Macrosiphini.

In a revision of four Eurydema speices recorded in Far East Asia, we confirm only two species, one of which consists of two subspecies: E. dominulus (Scopoli 1763) [=E. pulchra (Westwood 1837), syn. nov.], E. gebleri gebleri Kolenati 1846, and E. gebleri rugosa Motschulsky 1861 [stat. nov.]. In order to prove the above taxonomic changes, we compared three major characters; (1) the color patterns, (2) the mitochondrial COI (DNA barcoding) and (3) cross– breeding fertility (inter–specific copulation). Two subspecies, E. g. rugosa and E. g. gebleri, preserve their own unique coloration patterns, confirmed by the intra–subspecific copulation and breeding. Interestingly, the 1st progeny from the inter–subspecific copulation of E. g. rugosa♂ X E. g. gebleri♀ (or E. g. gebleri♂ X E. g. rugosa♀) take the coloration patterns inherited from E. g. gebleri.

In traditional taxonomy on the family Cantharidae, color pattern of the body and the structure of the male genitalia have been often used as diagnostic characters in identification of the specific level. However, these characters caused the difficulty in identifying the female in case a species was described only by male specimens or has the several color types among individuals. In this study, we attempted to evaluate the species reality of Asiopodabrus fragiliformis which was often difficult to be identified due to individual variation in color pattern and lack of information of female, through searching for new morphological diagnostic characters as well as DNA barcoding analysis, including their closely relative species from Russia and Japan. The results showed that A. fragiliformis was represented as three clusters strongly supported by high value of boots trap (>99%) and over 3% branch length. The pairwise distances between species of Asiopodabrus were detected larger, ranged from 3.4–9.5%, than the intragroup distance ranged from 0–2.9% indicating presence of a barcoding gap. And then, the three clusters were respectively determined as A. fragiliformis, A. kurvatovi and a new species through the analysis of morphology and COI gene. Therefore, we suggest that the species delineation on polymorphic species and the female specimens of closely resembling species would be more exactly and effectively determined if DNA barcoding and the traditional taxonomy are used as complementary methods for identification.

We present results of a H13CN J=1-0 mapping survey of molecular clouds toward the Galactic Center (GC) region of -1.6° ≤ l ≤ 2° and -0.23° ≤ b ≤ 0.30° with 2' grid resolution. The H13CN emissions show similar distribution and velocity structures to those of the H12CN emissions, but are found to better trace the feature saturated with H12CN (1-0). The bright components among multi-components of H12CN line profiles usually appear in the H13CN line while most of the dynamically forbidden, weak H12CN components are seldom detected in the H13CN line. We also present results of other complementary observations in 12CO (J=1-0) and 13CO (J=1-0) lines to estimate physical quantities of the GC clouds, such as fractional abundance of HCN isotopes and mass of the GC cloud complexes. We confirm that the GC has very rich chemistry. The overall fractional abundance of H12CN and H13CN relative to H2 in the GC region is found to be significantly higher than those of any other regions, such as star forming region and dark cloud. Especially cloud complexes nearer to the GC tend to have various higher abundance of HCN. Total mass of the HCN molecular clouds within |l|≤ 6° is estimated to be ~2 ×10 7 M⊙ using the abundances of HCN isotopes, which is fairly consistent with previous other estimates. Masses of four main complexes in the GC range from a few 10 5 to ~ 10 7 M⊙ All the HCN spectra with multi-components for the four main cloud complexes were investigated to compare the line widths of the complexes. The largest mode (45 km s-1) of the FWHM distributions among the complexes is in the Clump 2. The value of the mode tends to be smaller at the farther complexes from the GC.